R     And    S5/4.5e.
S     And    SN (NGC 224).
W     And    S7.5/1-e.
X     And    S5/7-e.
Z     And    The light curve is characterized
             by outbursts up to 4m with intervals of 10 - 20
             years. In the intervals cyclic variations are observed with
             the mean period of 632d and variations with cycles of
             several days and Delta(m) ~ 0.1m - 0.5m. The spectrum is
             symbiotic, with features of a late M giant, narrow
             low-excitation emission lines (Bleq) and forbidden lines
             characteristic of highly excited nebulae.
RR    And    S6/3.5e.
RT    And    Min II 8.88; DI = DII = 0.17P; dI = dII = 0.00. P var.
             Nonlinear term: -6.33*10**(-11)*E**2. During
             JD2433477 - 43878 linear elements are satisfactory:
             Min = 2441141.8888 + 0.62892984d*E. Period changes
             according to a sine law are possible [08002].
RU    And    P var. Max = 2419857 + 243.0d*E (JD2412800 -
             20000); Max = 2434551 + 233.24d*E (JD2420000 -
             34550). Since JD2435000 - see Table. Delta(m) ~ 4m - 5m
             (before JD2429600), ~1m (JD2429600 ~ 33600), up to 3m
             (JD ~2436000),  ~1.5m (JD ~2436700). In 1970 - 1972
             showed quite irregular variations.
RX    And    SB (P = 0.21173d). Cyclic variations with P ~ 38s - 54s
             were observed after a normal maximum; after a short
             maximum no periodicity was found [08004].
SS    And    Two long period variations are also observed:
             P = 650d, P = 3800d.
ST    And    P var. Max = 2418370 + 337.3d*E (JD2418000 - 28000).
             Since JD2428000 - see Table.
SU    And    VB A (B 12.77m V, F0V:, 15").
SV    And    The magnitude in Max varies periodically, P = 930d,
             P = 5400d? [02146].
SW    And    [Fe/H] = +0.16. P var. Nonlinear term:
             -1.229d*10**(-10)*E**2 [01959]. Since 1959
             Max = 2436466.828 + 0.442270121d*E [06929].
             The shape of the light curve varies with
             Pi ~36.83d = 83.28 P. The deviations (O - C) satisfy
             the elements of Blazhko effect
             Max(O - C) = 2436816.23 + 36.921d*N. Secular trend
             and cyclic (P ~2a) variations of (O - C) are possible
             [08005].
SY    And    d = 0.027P.
TT    And    Min II 11.6?
TU    And    P var (Pi ~37a?).
TV    And    P var? Delta(m) strongly varies.
TW    And    d = 0.020P. Min II 8.94. P var. Min = 2428845.422 +
             4.122739d*E (JD2420050 - 32000). Since JD2432000 - see
             Table.
TZ    And    P1 = 118d: [00882].
             Mean magnitude varies with P2 = 974d [00098]. P = 135d
             (JD2437545 - 38377) [03367].
UU    And    P var. Min = 2428832.536 + 1.486311d*E (JD2421455 - 23740)
             [02262]; Min = 2428832.465 + 1.48629d*E (JD2428830 - 35012)
             [00745]. Since JD2441100 - see Table.
UW    And    P var. Before JD2430000 Max = 2418585 + 236.7d*E. Since
             JD2436000 - see Table.
WW    And    d = 0.012P.
WX    And    P var. Max = 2422613.614 + 3.0012544d*E (JD2422610 - 34712)
             [01240]. The Table gives current elements. d = 0.03P
             in 1972 and probably varies.
WZ    And    Min II 11.9. P var [02262]. Min = 2435075.342 + 0.695662d*E
             (before JD2440500); probably
             Min = 2440872.290 + 0.6956576d*E since JD2440500.
             The elements in the Table represent all the observations
             satisfactorily.
XX    And    P var. Max = 2418001.938 + 0.7227486d*E (1908 - 1932);
             Max = 2427106.403 + 0.7227591d*E (1932 - 1946) [02264].
             Since 1946 - see Table. Delta(S) = 9. Blazhko effect:
             Max = 2437578 + 36d*N [03111].
XY    And    Blazhko effect is possible.
XZ    And    Min II 10.16; DII = 0.26P. P var [02431, 06932, 08008,
             08593]. Min = 2432883.6046 + 1.3572708d*E (JD2431700 -
             36150) [01977]; Min = 2441954.340 + 1.357293d*E
             (since JD2436200). The elements in the Table represent all
             the observations satisfactorily.
AA    And    Min II 10.5.
AB    And    Min II 10.20. P var. Period increased suddenly in 1953
             ( ~JD2434500); no period changes later [02509, 05222].
             Elements since 1953 - see Table.
AC    And    Unusual multiperiodical variable. Second oscillation:
             Max = 2432467.373 + 0.71124243d*E; P3 = 0.421069d [08187],
             see also [08294, 08295]. Delta(S) = -1:.
AD    And    Min II 11.6. Depth of minima in yellow light: 0.62m (Min I),
             0.58m (Min II) [03141]. Min II - Min I = 0.494P. P var.
             Min = 2428718.402 + 0.9861940d*E (JD2417460 - 29640)
             [01983]. Since JD2428700 - see Table.
AE    And    In the M31 galaxy. Strong UV continuum.
             Emissions: H, He I, Fe II, [Fe II].
AF    And    In the M31 galaxy. Strong UV continuum.
             Emissions: H, He I, Fe II, [Fe II].
AG    And    According to [08296], DSCT:, Min = 2442636.5868 + 0.0347d*E,
             A = 0.5m.
AM    And    VB A (B 0.25' S).
AN    And    Min II 6.09. The existence of the third body in
             the system is possible. Sp(Met) = F2 - F5.
AP    And    Min II 11.9. The period may be 2 times shorter.
AT    And    B - V: +0.42, +0.56. Delta(S) = 3. See [08299] for data
             on period variations and a detailed study.
BD    And    Min II 11.4.
BE    And    Average cycle: 137d [01993, 02267]; 156.8d after JD2431700.
BL    And    Depth of Min II 0.24m: P var? Min I = 2429491.255 +
             0.7223779d*E (JD2415800 - 33900) [01995]. Since JD2433900 -
             see Table.
BX    And    ADS 1671 A (B 9.7m, 20", 59deg). Min II 9.15. Possible
             period change from 0.61011222d to 0.61011534d (~1952).
             On the period changes see also [08657].
BY    And    According to [08658], SRB:.
CC    And    Possibly in a binary with Porb = 10.469d. Delta(m) and the
             light curve shape vary with a period 5.23714d or 10.469d
             [08016]. According to [03120], 4 periods are present:
             P2 = 0.0632083d. First overtone was not found. Other
             periods are resonances.
CG    And    P var: 3.7430d (1950), 3.7394d (1963) [05224].
             Cyclic period changes are possible.
             According to [06941], short period oscillations (P = 2h 04m)
             are present. A number of observers do not find short-term
             variability.
CM    And    According to [00821], Max = 2428380 + 140d*E and Max =
             2430616 + 124d*E, and the star resembles UU Her.
CN    And    Min II 9.96.
CO    And    d = 0.06P:
CP    And    d = 0.01P? Depth of Min II 0.05m?
CU    And    d > 0.034P ([06943], according to visual observations.)
DI    And    DCEP? [03165].
DK    And    EW?
DL    And    In the field of the open cluster NGC 7686.
DR    And    P var. Before ~JD2437000 Max = 2436078.384 + 0.5630609d*E
             [02275]; then P changed abruptly. Delta(m) changes by ~0.3m,
             Max A1 = 2436078.8 + 69.486d*N1, Max A2 = 2437646.65 +
             69.719d*N2. Other possible cycles are 2000d (interaction
             of cycles N1 and N2) and ~30 years [08019].
DS    And    In the field of the open cluster NGC 752. Min II 10.7.
DZ    And    According to [04008], type RCB, spectrum R. According to
             [06945], since 1961 is in Max light all the time. According
             to [06946], the spectrum is not characteristic of RCB stars.
             According to [08660], the star was bright near the moments
             of Min light given in [04008].
EG    And    P = 40d or 80d [08020].
             Absorption spectrum with overlaying emissions of high
             excitation [04434, 08598]. Strong variable magnetic field
             [04435]. Long period variations of light are observed.
             Radial velocities profiles and equivalent widths of lines
             vary with P = 470d [08596] (SB? [08597]). Possibly is
             analogous to HM Sge [08598].
EH    And    IR excess. The presence of a dust envelope is possible.
EO    And    Very red.
EP    And    Min II 12.5.
ET    And    Delta(B) = 0.035m, Delta(U) = 0.07m.
             The Table gives the epoch of Max light. Observations may
             be represented by the periods 0.723d and 1.61553d
             [08022, 07946]. According to [08023], in June - December 1977
             Min = 2443337.4725 + 0.49925d*E, other periods are
             not satisfied by observations. According to [08599],
             Max(U) = 2439751.28 + 0.617135d*E (1967 - 1971).
             SB, Max(Vr) = JD2443718.0 + 48.304d*E [08301].
             Photometric periods could not be found in radial
             velocities.
EX    And    Possible Min II 13.0:, Min II - Min I = 0.55P.
EY    And    I - K = 5.38;
             the presence of a dust envelope is possible [06947].
FF    And    10.35m - 10.42m V outside flares;  M - m = 0.50P.
             Porb = 2.170304d [08024]. According to photometric
             observations, P = 2.14d (1971), P = 2.15d (1972),
             P = 2.19d (1973) [06948].
FG    And    According to [04156], EA; Min = 2436074.528 + 0.99772d*E.
FL    And    d = 0.02P.
FZ    And    mu = 1", p = 64deg.
GK    And    Min II 11.5.
GN    And    ADS 409 A (B 13.3m, 2", 6deg; C 11.6m, 141", 130deg).
             Different authors give spectral types F0 III, F2V, Am
             (probably based on different criteria).
GP    And    Delta(m) changes with P2 = 0.64d.
             A wave with P3 = 0.012161d is present. The mean
             magnitude and the shape of the light curve vary
             [08302].
GQ    And    ADS 246 B (A = GX And; B 37", 61deg). B - V = +1.80.
             X-ray source.
GR    And    Min (magnet.field) = 2442288 + 525d*E.
             Magnetic field varies (-250 to -1030 Gauss). Period of
             changes of C1 is near 1.5 years [07893]. According to [06257],
             period of changes in u is near 1 year or longer.
GS    And    B - V = +1.7 in normal light.
GX    And    ADS 246 A (B = GQ And, 37", 61deg). Delta(U) = 0.55m. SB?
             (conflicting data).
GY    And    SB1 (P = 273.2d [07324], P = 272.99d [08303]).
             For spectral changes, variations of light and magnetic
             field it is possible that P = 23a [07004] or 20.60a [08303].
             [08022] gives P ~36.5d and Delta(V) ~0.049m. Periods 4.92a
             and 1.8d may exist [08303].
GZ    And    B - V: +0.77, +0.82. ADS 1693 A (B 11.13m, 8", 31deg).
             Min II 11.58. P var?
             The period is based only on Minima I [06830] and
             was improved with account of recent data.
HH    And    Subdwarf? [06581]. mu = 1.82", p = 176deg.
HI    And    B - V = 1.8m outside flares.
HN    And    Max(U) = 2438327.8 + 69.433d*E [08022]. SB
             (P = 106.27d [07435]).
HQ    And    According to [08659], a probable cataclysmic binary;
             similarity to AM Her and AN UMa is noted.
HR    And    d = 0.05P.
HT    And    B - V = +0.60. In the region of M 31.
HU    And    Min II 17.2. In the region of M 31.
HV    And    According to [08659], a probable cataclysmic binary;
             similarity to AM Her and AN UMa is noted.
HY    And    In the region of M 31.
HZ    And    In the region of M 31. P > 100d. Red.
IL    And    d = 0.02P.
IM    And    In the region of M 31.8.
IO    And    According to [08659], a probable cataclysmic binary;
             similarity to AM Her and AN UMa is noted.
IP    And    d = 0.02P:.
KK    And    The light curve has double-wave shape
             [07740]. Long period variations were found [07955].
KU    And    I - K = 4.63.
             SR type is possible. Surrounded with a dust envelope [08029].
KX    And    SB2 (P = 38.908d).
KZ    And    ADS 16557 B (A 7.0m; B 15", 254).
LM    And    Min II 12.7.
LN    And    Delta(B) = 0.025.
LO    And    Min II 11.82.
V0369 And    VB (0".1, 128 deg, 1986.9).
V0374 And    Not identical with BD+44 422.
alf   And    SB (P = 96.6960d). VB A (B 11.2m, 80").
             Epoch of Max U light is given.
             Hbeta index varies in the range of ~0.02m with P
             ~3h [08030]. Rapid rotation.
zet   And    Depth of Min II 0.1m. SB.
             Unstable light curve. Most notable
             variations on the rising branch of Max II [08030].
             Many peculiarities in the spectrum.
lam   And    SB1 (P = 20.52d).
omi   And    v sin i = 300 km/s; VB(0.3"; possibly
             also 0.05" - according to speckle-interferometric data).
             Shell spectrum appeared and disappeared several
             times since 1890. Different authors attributed
             the star to EB type. According to [05955], The changes
             of light may be explained also by intrinsic
             variations of a single shell star. They are represented
             by elements: Min I = 2439470.628 + 1.0185d*E.
             According to [02572], Min I = 2436174.430 +
             1.5998398d*E. The periodogram analysis shows
             a stable peak at P ~0.84d [08032]. A possible shell
             event was observed late in 1975.
S     Ant    Min II 6.87. P var?
T     Ant    CWB? P var. [A/H] =  -0.0. P = 5.9098d (JD2428187 -
             34688), P = 5.8976d (JD2434688 - 37660) [05387].
             The Table gives mean elements which satisfy all
             observations well enough.
V     Ant    OH, H2O maser.
Z     Ant    Mean brightness varies with P = 1143d.
SW    Ant    Min II 14.6.
UZ    Ant    P var?
WY    Ant    P var. P = 0.57430871d (JD2414000 - 22070); P =
             0.57431618d (JD2422070 - 25600); P = 0.57431216d
             (JD2425600 - 29000) [01113]. (k - b)2 = 0.00.
WZ    Ant    Min II 11.8.
XX    Ant    Min II 9.1.
XY    Ant    Depth of Min II 0.3m - 0.5m pg.
XZ    Ant    Min II 10.2.
Z     Aps    Possibly also an eclipsing binary.
RT    Aps    Strong variations of period and the shape of
             the light curve [06152].
TY    Aps    Delta(S) = 3.
YY    Aps    The period is probably long.
AF    Aps    Min II 13.9.
AN    Aps    Min II 12.8.
AP    Aps    Min II 15.5.
AS    Aps    Min II 13.8.
AV    Aps    Depth of Min II 0.05m.
CE    Aps    P = 209d or 261d.
CY    Aps    Min II 13.0.
EF    Aps    Min II 12.6.
FY    Aps    Deep Min II.
GK    Aps    Min II 13.9. RRC type is possible.
GO    Aps    Min II 14.8. RR type is possible.
GQ    Aps    Min II 14.8.
GU    Aps    Min II 14.5.
GX    Aps    RV type is not excluded. The epoch of Min is given.
GY    Aps    Min II 14.2.
HL    Aps    Min II 12.6.
HO    Aps    Min II 13.7.
HT    Aps    Min II 14.3.
HV    Aps    Epoch of Min is given.
HX    Aps    Min II 14.4.
II    Aps    Min II 11.6.
IL    Aps    Epoch of Min is given.
IO    Aps    Min II 12.4.
IR    Aps    Min II 13.8.
IU    Aps    Min II 14.6.
IY    Aps    Min II 12.9.
KN    Aps    d ~0.03P.
KR    Aps    Possibly a slow eclipsing variable.
KT    Aps    Min II 15.2.
KV    Aps    Min II 13.6.
KZ    Aps    Smooth light
             changes with superimposed variations of eclipsing
             nature, with minima on JD2436729 and 2436808.
LM    Aps    RV type is possible.
LN    Aps    Min II 13.3.
LO    Aps    Min II 11.5.
MY    Aps    L19-2. P0 = 192.75s, P1 = 113.77s.
del 1 Aps    In a wide pair (delta2 Aps, 100", common mu).
kap 1 Aps    SB? VB A (B 11.27m V, 27").
R     Aqr    Symbiotic spectrum. Emissions of H, SII, OIII, FeII, NeIII,
             OII. Variable radio source. SiO maser. The secondary may
             be an accreting white dwarf. The star is embedded in an
             expanding gaseous nebula several hundred years
             old. A cycle ~24a and longer-term variations are
             possible in the changes of radial velocities and period.
U     Aqr    Strong bands of 12C2, CN,
             lines of SrII, YII in the spectrum; hydrogen deficiency.
             A probable halo star (Vr ~100 km/s.).
Z     Aqr    1969 - 70: P = 100d +- [05973].
RY    Aqr    P var. Min = 2433872.352 + 1.966598d*E (before
             JD2428000); Min = 2440824.410 + 1.966620d*E
             (JD2428000 - 41000); Min = 2440824.410 +
             1.966611d*E (JD2441000 - 43800). Since
             JD2443800 P = 1.966554d?
             The Table gives elements representing
             observations after JD2428000 with the accuracy +-0.1d.
ST    Aqr    Min II 9.37. P var. Min = 2423640.271 + 0.78101367d*E
             (JD2423500 - 26000) [02037]. Since JD2439700 - see Table.
SU    Aqr    ADS 16318 A (B 10.7m, 5", 144deg). Min II 10.5. P var?
SV    Aqr    Cycle 200 - 300d is possible.
SW    Aqr    P var. (k - b)2 = 0.01.
SX    Aqr    P var? Delta(S) = 9.
SZ    Aqr    Epoch of Min is given.
TT    Aqr    VB A (B 15m, 3", 135deg).
TZ    Aqr    Delta(S) = 5.
VY    Aqr    Second outburst: Max ~JD2437897
             (1962),  ~9m pg [03129].
WX    Aqr    Blazhko effect is possible.
XZ    Aqr    P var. Before JD2437913 P = 2.059187d.
YZ    Aqr    B - V = 0.49 (in Min). (k - b)2 = 0.06.
             Small fluctuations of period are possible.
AE    Aqr    Unusual flare X-ray system with pulsar. Becomes bluer
             in Max. In Min B - V = +0.92. Shows rapid irregular
             variations, which differ it from UV stars and UG
             system, though the spectra are somewhat similar.
             Simultaneous photoelectric and spectroscopic observations
             [03131] show the existence of two types of flares:
             1) intensification of emission lines accompanied by
             brightening in U and B; 2) intensification of continuum
             leading to brightening in U, B and V ("white flare").
             Detailed spectroscopic investigation [01971].
             Porb = 0.41165794d + 1.12*10**(-10)*E, The epoch
             T0 = JD2439030.621 [08672]. In the X-ray band
             (0.1 - 4.0 keV) pulsations with P = 33.0767s are observed
             [08673]. In the optical range pulsations with
             P0 = 33.076737s as well as with P1 = 16.5s were noted
             [08674, 08675].
AT    Aqr    Min II 14.7.
AX    Aqr    P var. Before ~JD2427367 Max = 2425417.60 + 0.388135d*E
             [03113].
AY    Aqr    Min II 14.3.
BH    Aqr    P var. Before ~JD2431150 Max = 2426948.411 + 0.5258022d*E
             [03113].
BI    Aqr    Min II 13.1.
BK    Aqr    Close companion.
BL    Aqr    Waves from 80 to 125d. Mean magnitude changes
             with cycles from 480 to 700d in the range of 0.3m - 0.6m.
BM    Aqr    The mean magnitude may vary with P = 500 - 600d.
BN    Aqr    Delta(S) = 4:. P var. Before JD2428964 Max =
             2426577.901 + 0.46963401d*E [03113].
             According to [05391] Max = 2429395.742 +
             0.4696410d*E + 3.3*10**(-10)*E**2 (1898 - 1958).
BO    Aqr    P var? (k - b)2 = 0.01.
BQ    Aqr    d = 0.07P.
BR    Aqr    P var? (k - b)2 = 0.16.
BS    Aqr    Delta(S) = 0. P var?
BT    Aqr    B - V: +0.14, +0.52. P var. Blazhko effect.
BV    Aqr    P var. Blazhko effect with Pi =  11.56d and variations of
             light in Max up to 0.75A.
BW    Aqr    d = 0.01P. Min II 10.8. Min II - Min I = 0.484P.
             Jensch [00189] considers the secondary Min to be the
             main one.
BX    Aqr    d = 0.027P.
CD    Aqr    d = 0.012P. Min II 10.2.
CE    Aqr    According to [02548], no
             variations were found in visual observations during
             several months in 1954 - 1958. According to [03138],
             the star may be analogous to AI Vel; P = 0.16d?
CH    Aqr    P var?
CI    Aqr    Period may be twice as long.
CM    Aqr    Min II 13.6.
CP    Aqr    Delta(S) = 3.
CR    Aqr    Min II 14.2.
CV    Aqr    Minor planet (52) Europa.
CW    Aqr    Min II 10.8.
CX    Aqr    Min II 10.8. Broad hydrogen lines.
CY    Aqr    Delta(S) = 2. P var; abrupt change ~1952. Before JD2434000
             Max = 2434308.4314 + 0.061038509d*E. The shape of
             the light curve probably varies. For M - m different
             authors give values from 0.23p to 0.40p. Beat phenomenon
             with P2 = 0.2182d is possible [08060].
CZ    Aqr    Min II 11.1. Cyclic variations of period?
DD    Aqr    Min II 11.2.
DN    Aqr    (k - b)2 = 0.01.
DO    Aqr    P var.
DS    Aqr    P var.
DV    Aqr    Min II 6.1. SB. In [08061] variations were noted
             with Delta(m) ~0.1m and P < 3h, presumably of DSCT
             type nature. Some sources give A3 for the spectral
             type. Shell spectrum was observed in May, 1975.
             Spectral lines were filled with emission and therefore
             weak, strong absorption in H and K CaII lines was present.
             Shell effects were not present in the spectra taken in
             1971 - 1973 [08062].
DX    Aqr    VB B (A 7.0m, K0III; B 3.7", 244deg). SB1. d ~0.015P.
             Depth of Min II ~0.3m.
             The range of combined brightness is given.
DY    Aqr    d = 0.04P.
EE    Aqr    Min II 8.48.
EK    Aqr    Min II 11.23.
EL    Aqr    P = 0.6345d is possible.
EM    Aqr    According to [06204] P = 0.068d.
             Period and amplitude vary on very short time
             scale. Light and colour vary approximately in phase.
             The beat period, if exists, is shorter than 1d.
ET    Aqr    Period is given according to [08336].
EW    Aqr    Delta(m) varies.
FF    Aqr    d = 0.059P. SB1. The unique eclipsing system of a red
             star and probably a blue hot subdwarf. The amplitude of
             the eclipse is 0.15V, 0.4B, 1.2U. The magnitude in Max
             varies by 0.35V, 0.33B, 0.22U. Variable shape of light
             curve. Strong emissions H and K CaII, Halpha in the
             spectrum.
FI    Aqr    Possibly P = 4.659d or 4.719d. Epoch of min is given.
FK    Aqr    BDS 11854 A (B = FL Aqr, 11.45m, 24", 352deg, 1966).
             mu alpha = +0.455", mu delta =  -0.067". SB2 (P = 4.08322d
             [00313]). Flares Delta(U) = 0.7 [00344].
FL    Aqr    BDS 11854 B (A = FK Aqr; B 24", 352deg, 1966).
KV    Aqr    One deep fading overlapping a brightening trend.
omi   Aqr    Shell or disk spectrum is observed.
pi    Aqr    The brightness increased by ~0.2m V
             in 1957 - 1975, the star became redder. Balmer
             continuum in emission. Rapid changes in emission
             lines and in polarization. Existence of a disk
             or a shell is possible.
R     Aql    P var. Max = 2440038 + 297d*E (JD2427850 - 40000).
             Since JD2440000 - see Table.
             For the whole observed period
             Max = 2399190 + 346.932d*n - 0.239303d*n**2;
             Pn = 348.980d - 0.554202d*n + 0.000552309d*n**2 [03143].
             H2O, OH and SiO maser. Radiobursts.
U     Aql    B - V: +0.84, +1.24. P var. ADS 12503 A (B 14.00m,
             35", 349deg, 1900; one more companion 11.7m V, 2", 230deg,
             1934).
W     Aql    S 6/6e. Composite spectrum near Min light; a companion
             (F5 - F8) may exist [03502].
Y     Aql    Depth of Min II 0.03m. SB1.
RR    Aql    Maser H2O, OH, SiO.
RT    Aql    Maser H20, OH, SiO.
SY    Aql    Maser H2O, OH.
SZ    Aql    B - V: +1.04, +1.82. P var [02392]. Before JD2420260
             P = 17.1359d. Current elements - see Table.
TT    Aql    B - V: +0.96, +1.62. P var. [02392]. Before JD2418035
             P = 13.7518d.  Current elements - see Table.
TV    Aql    P var (changed at ~JD2430000).
             Before JD2430000 Max = 2429730 + 237.9d*E.
TW    Aql    Cycles 65d or 95d are observed during different time
             intervals [08714].
UU    Aql    Mean cycle: 71.3d [04063]; 56d [03144].
UY    Aql    Cyclic changes of light (P ~400d) with superimposed very
             rapid variations are noted in [00504].
VX    Aql    SC5-/8e. According to [04231], the variable is irregular.
             Lithium star.
VZ    Aql    B - V: +0.61, +1.01.
XZ    Aql    P var. Min = 2424449.277 + 2.139147d*E
             (JD2424380 - 2430300). Since JD2433000 - see Table.
YZ    Aql    d = 0.03P. P var.
AA    Aql    Delta(S) = 1.0.
AC    Aql    P var.
AD    Aql    CN bands are observed in the spectrum. According to [06928],
             the range is 8.83 - 13.42 V.
AE    Aql    VB A (B 16.6m, 12", 330deg; C 16.9m, 11", 0deg).
             The combined light of A, B, C varies in the range
             13.9 - 15.8.
AF    Aql    The period may be two times shorter.
AL    Aql    d = 0.04P.
AU    Aql    According to [03146], P = 190d or 380d.
BL    Aql    P var. Max = 2418538 + 159.65d*E (JD2418529 -
             29075). During JD2436420 - 38940 - see Table.
BY    Aql    P var?
CD    Aql    Close companion?
CL    Aql    Sometimes maxima predicted according to the
             elements do not occur.
CM    Aql    Symbiotic spectrum similar to that of Z And [03149].
CR    Aql    Considerable Blazhko effect is possible.
CS    Aql    Close companion?
CT    Aql    According to [06004], only slow irregular variations with
             Delta(m) ~0.6 were observed in 1963 - 1968.
CU    Aql    P var? (Possible change ~JD2423000). Earlier Max = 2418591
             + 203.7d*E.
CV    Aql    P var?
CW    Aql    Close companion?
DD    Aql    Close companion?
DT    Aql    P var (Change ~JD2425000). Earlier Max = 2423964 + 290.5d*E.
DY    Aql    P var [06107].
EV    Aql    P var. Before JD2423900 P = 38.67d. [A/H] = -0.3.
EX    Aql    P = 117d is also observed.
EZ    Aql    P var [06107].
FF    Aql    ADS 11884 A (B 10.37m, 7", 141deg). SB1 (P = 1435d).
FG    Aql    At the edge of the dark nebula Barnard 130. May be a
             physical pair with FH Aql (rho ~20"). According to
             [00504], the mean cycle of light variations is 3.5d.
             The level of mean light varies.
FH    Aql    At the edge of the dark nebula Barnard 130. May be a
             physical pair with FG Aql (rho ~ 20"). According to
             [00504], the mean cycle of light variations is 3.44d.
FK    Aql    Depth of Min II 0.03m. P var.
FM    Aql    B - V: +1.12, +1.50.
FN    Aql    B - V: +1.10, +1.39. P var.
FZ    Aql    VB A (B 11.5m, 14", 162deg).
GM    Aql    UV type is possible [00504].
GU    Aql    d = 0.02P.
GV    Aql    Nova-like star according to [02089].
GY    Aql    Maser OH, SiO.
HK    Aql    Type ISB is not excluded.
HL    Aql    P var? The 15m star shown in the charts [02274, 06996] with
             co-ordinates coincident with those given at the discovery
             is constant according to [02274].
IM    Aql    P var. Before JD2432772 Max = 2428064.707 + 0.4569602d*E.
IO    Aql    VB A (B = IP Aql, 30", 101deg).
IP    Aql    VB B (A = IO Aql).
IS    Aql    Close companion.
KL    Aql    B - V: +0.78, +1.19, [A/H] = 0.6.
KO    Aql    d = 0.018P. Min II 8.40. P var. Min = 2427550.565 +
             2.863859d*E (JD2426250 - 33000) [02462]; Min =
             2433888.366 + 2.863954d*E (JD2433000 - 39000).
             current elements - see Table.
KP    Aql    Min II 10.43; Min II - Min I = 0.50P; DII = DI.
KV    Aql    During JD2429130 - 31370 - see Table.
             During JD2428308 - 28433 the star was faint. Max 2436015
             also is not satisfied by the elements.
LU    Aql    In [03158] P = 102d is given, and the existence of the
             variation of mean magnitude with P ~1080d and
             Delta(m) = 0.4m was suspected.
MV    Aql    Close component, the range is given for combined light.
NN    Aql    Cyclic P variations?
NV    Aql    Variations of mean light with P ~ 900d - 1000d and
             Delta(m) ~0.6m.
OO    Aql    Min II 9.8. P var. Min I = 2426892.0582 +
             0.5067954d*E (1932 - 1934), Min I = 2433925.3762 +
             0.5067943d*E [08072]. Since JD2438000 - see Table.
             The shape of the light curve varies.
OX    Aql    Var 2 in the chart for OW Aql.
PP    Aql    [A/H] = -0.0. CWA type
             is not excluded. According to [03161]
             P var. Max = 2415229.15 + 24.0147d*E (JD2415228 -
             21064), Max = 2426576.14 + 24.074d*E (JD2426576 -
             29489). After JD2432040 Max = 2433141.78 + 23.994d*E.
             Current elements Max = 2436836.04 + 23.973d*E.
PZ    Aql    P var? According to [05387], before JD2428075 P = 8.7555d;
             P = 8.7504d (JD2428075 - 34725); since JD2434725
             P = 8.7573d. See also [02274]. Elements in the Table are
             satisfactory after JD2433150. The shape of the light curve
             apparently varies.
QS    Aql    Min II 5.97. VB (A 6.5m; B 6.7m, 0.18", 137deg). P var.
QV    Aql    The epoch of main Max is given.
QY    Aql    d = 0.016P. P var?
V0336 Aql    B - V: +1.17, +1.55.
V0337 Aql    Min II 9.09. P var.
             The shape of the light curve varies.
V0340 Aql    d = 0.05P. P var.
V0341 Aql    P var. Delta(S) = 4.
V0342 Aql    ADS 12259 B (A 7.5m; B 20", 14deg); d = 0.032P. P
             increases (see also [02265, 04493]). Before JD2435600 Min =
             2428023.550 + 3.390842d*E.
             Halpha emission observed at Max light [08074]. The shape
             of the light curve and d apparently vary. Delta(m)
             probably decreases [08075].
V0343 Aql    Min II 10.7.
V0346 Aql    Min II 9.1. ADS 13438 A (B 11.3m, 2", 245deg).
             Elements in the Table are valid after
             JD2437000. The shape of Min I varies [07001].
V0348 Aql    d ~0.08P.
V0352 Aql    The nucleus of the supposed planetary nebula P.K.
             37-3.3deg.
V0356 Aql    VB A (B 0.2").
V0367 Aql    The elements are satisfactory
             only during JD2436450 - 37960. Resembles S Vul.
V0368 Aql    VB A (B 0.17", 140deg).
V0374 Aql    VB A (B ~0.2',  ~270deg).
V0406 Aql    Min II 13.3:.
V0407 Aql    P var; there is a nonlinear term in the elements:
             +1.51d*10**(-9)*E**2.
V0409 Aql    Min II 12.2. Spectral type from another publication
             is A2 - A3.
V0411 Aql    Epoch of Min is given.
V0417 Aql    Min II 11.5. P var. Before JD2439000:
             Min = 2428427.127 + 0.3701251d*E.
V0421 Aql    P var?
V0423 Aql    Elements are valid for JD2426900 - 28000. During
             JD2429020 - 31670 the waves are much longer or absent.
V0433 Aql    Waves of 26d - 80d duration with Delta(m) = 0.1m - 0.9m.
             The mean light varies according to the formula
             Max = 2438312 + 648d*E.
V0449 Aql    The star in [01091, 02282] is actually not identical to HV5424.
V0461 Aql    Close component ~15.5m, the range of combined light is
             given.
V0467 Aql    Waves of 40d - 72d duration. The mean light varies with
             P ~1400d.
V0473 Aql    P ~330d is sometimes observed.
V0476 Aql    EW type with doubled period is possible. Elements are based
             on a short series of observations.
V0483 Aql    In the field of the open cluster NGC 6709.
V0486 Aql    In the field of the open cluster NGC 6709.
V0493 Aql    B - V: +1.10, +1.38.
V0495 Aql    d = 0.06P:.
V0496 Aql    B - V: +1.07, +1.28. Elements are given for epochs after
             JD2428000.
V0497 Aql    VB A (B 16.5m, 9",  ~0deg).
V0524 Aql    The variable is np from the star shown in the chart
             in [02317].
V0527 Aql    IS type is possible.
V0528 Aql    VB A (B 16.5m, 11", 59deg).
V0535 Aql    VB [01943], two components are seen on Palomar prints,
             eastern of them being red. According to [01943], rapid
             variable.
V0537 Aql    Possible P = 200d.
V0538 Aql    Possible P = 375d.
V0558 Aql    Possible P = 187d.
V0571 Aql    Possible P = 185.5d.
V0572 Aql    B - V: +0.65, +0.87. P var. Before JD2435500 P ~3.7686d.
             See also [08637]. JD2433631.8421 + 0.716292d*E.
             See also [02124].
V0586 Aql    Irregularities are sometimes observed, but then the
             periodicity is probably resumed.
V0596 Aql    Resembles S Vul.
V0599 Aql    Min II 6.73. According to [08083], may be constant.
V0600 Aql    B - V: +1.36, +1.70.
             Before JD2428000 another value of P is possible [08632].
V0602 Aql    d = 0.02P. Min II 12.7.
V0603 Aql    SB (P = 0.13854d [03169]). Outside the outburst there are
             variations of light (eclipses) with Delta(m) = 0.30m,
             Min I = 2444401.399 + 0.1377d*E (D ~0.2P). The
             shape of the light curve and the depth of minima differ
             from cycle to cycle. The brightness in minima shows
             fluctuations apparently connected with the presence of
             a hot spot [04500].
V0605 Aql    A unigue variable. 8" np from a 17m star. Min ~20m pg.
             Photographs of the field [06041, 06042]. The
             light curve resembles those of the SN in NGC
             1058 or of eta Car [06040]. The only Max observed, with
             fluctuations, occured in 1918 - 1924. In 1921 the spectral
             type was found to be R [02464]. The star is inside the old
             planetary nebula A 58 and may be its nucleus.
V0609 Aql    Min II 11.9.
V0615 Aql    P var? Max = 2428046 + 364d*E (JD2428038 - 31343) [01091].
V0616 Aql    d = 0.04P. Elements reguire verification.
V0618 Aql    Twice shorter period is not excluded.
V0637 Aql    Twice shorter period is not excluded.
V0638 Aql    Twice shorter period is not excluded.
V0640 Aql    Min II 12.8.
V0647 Aql    Slight Min II [01091].
V0663 Aql    P = 194.5d is possible.
V0666 Aql    The range is given for combined magnitude with a preceding
             16.5m star. Separately was found ~17m pg near Min.
V0672 Aql    P var? Blazhko effect is possible [03113].
V0678 Aql    P var. Before JD2429723 Max = 2429723 + 120.6d*E.
V0688 Aql    Min II 10.8. DII = 0.15P.
V0694 Aql    d = 0.13P. VB (1"), a companion ~1m fainter than
             the variable [01881] may have affected the data given.
V0699 Aql    Min II 13.75.
V0706 Aql    Delta(S) = 0:.
V0708 Aql    P ~65d waves superimposed on slow variation of mean
             brightness with P ~1350d (JD2437124 - 40512) [06025].
             According to [00773] waves with P ~100d - 150d
             (JD2427543 - 31318).
V0714 Aql    d = 0.05P.
V0724 Aql    Min II 11.57.
V0733 Aql    P var? Before JD2434500,
             possibly Max = 2434453.72 + 6.17687d*E [00001].
V0734 Aql    VB A? (B 16.1m?).
V0743 Aql    White. SRD?
V0755 Aql    Alternative elements: Min = 2429195.290 + 1.01598d*E.
V0765 Aql    B - V: +0.70, +0.80.
V0766 Aql    EW type is not excluded.
V0769 Aql    d = 0.05P?
V0770 Aql    Min II 14.0.
V0771 Aql    According to [03165] UG.
V0774 Aql    Possibly resembles UV Boo.
V0777 Aql    P = 111.5d is possible.
V0784 Aql    Min II 14.8.
V0794 Aql    Rapid changes with Delta(m) up to 1.5m superimposed on
             slow ones. May belong to "polars" of XPRM type. Peculiar
             spectrum with broad emissions and blue continuum [08676].
V0800 Aql    VB. According to [06072] UGZ.
V0801 Aql    VB A (B 15.1m sp).
V0803 Aql    Min II 14.8.
V0804 Aql    Min II 12.8. In Max B - V = +0.61.
V0805 Aql    Min II 7.90, DII = 0.11P.
V0808 Aql    Min II 13.3.
V0812 Aql    VB A (B 16m sp, C 16m sf).
V0814 Aql    VB A (B 16.5m sp).
V0822 Aql    Min II 7.07. ADS 12538 A (B 10.1m, 1", 67deg). The shape
             of the light curve varies.(U - B) index in Min I is redder
             and Min II is bluer than average.
V0829 Aql    Twice longer P is possible.
V0836 Aql    RR type is possible ([00085]; it is suggested also by the
             spectrum [08676]).
V0850 Aql    In the centre of the planetary nebula P.K. 37-6.2.
V0866 Aql    Min II 14.8. According to [06026], the depth
             of Min II 0.4m, EB type.
V0867 Aql    P var?
V0871 Aql    Min II 14.5, Min II - Min I = 0.425P.
             Physical changes in the range 13.3 - 13.6 are
             possible. Eclipses start from the 13.6m level.
V0872 Aql    Min II 15.7:. Apsidal motion is possible.
V0873 Aql    P var? The mean light varies in the range 13.8 - 14.0.
V0875 Aql    White. According to [06004], rapid. Possibly UGZ or IA.
V0877 Aql    VB A (B 16.5m nf).
V0882 Aql    Blazhko effect is possible.
V0885 Aql    Min II 14.9:. Apsidal motion and changes of the shape of
             the light curve are possible.
V0888 Aql    A possible member of the open cluster NGC 6738.
V0889 Aql    Min II 9.0. Min II - Min I = 0.35P.
             Apsidal motion is possible.
V0890 Aql    Nova Aql 1946 = asteroid N258 Tyche [09038].
V0891 Aql    Min II 15.8.
V0895 Aql    P var. Max = 2430931.435 + 0.265108d*E
             (JD2426920 - 35010) [02267].
             During JD2441890 - 42290 - see Table.
V0907 Aql    Min II 15.7.
V0912 Aql    The shape of the light curve varies.
V0914 Aql    P = 3.336217d
             is given in [08717] by misprint.
V0919 Aql    Min II 13.8.
V0920 Aql    F or earlier observations Max = 2429458.400 + 0.4955033d*E.
V0922 Aql    Elements are not quite reliable.
V0923 Aql    Unusual shell star [01884]. Similar to EW Lac.
             He lines are widened by the rotation, NaI lines
             are narrow. Light changes are periodic: Min =
             2436458.66 + 0.8518d*E. The cause of variations is
             probably connected with the rotation and the inhomogeneous
             brightness distribution over the disk of the star [03178].
             Profiles of spectral lines vary. The expansion of the
             envelope terminated in 1965, which apparently led to the
             development of inhomogeneities and to the broadening of
             hydrogen line profiles [04525].
V0925 Aql    Some observers found constant brightness [03165].
V0929 Aql    Short period.
V0936 Aql    Short period.
V0947 Aql    According to [05412], rapid irregular
             changes are not excluded. According to [00504], constant.
V0955 Aql    Min II 14.9, DII = 0.13P.
V0956 Aql    Min II 14.2. Elements need confirmation.
V0957 Aql    P var. Max = 2428154.960 + 0.6051327d*E
             (JD2421871 - 28105).
V0958 Aql    VB A (B 17.0m, 0.2' np; C slightly brighter, 0.1'f).
             Combined magnitude of A and C is given.
V0964 Aql    Min II 13.7.
V0969 Aql    Blazhko effect is possible.
V0981 Aql    Min II 14.5.
V0991 Aql    IS type is possible.
V0992 Aql    According to [04260], P = 110d.
V0998 Aql    The position coincides with the planetary nebula
             P.K.50-3.1deg.
V0999 Aql    Tsessevich's observations [07806] do not agree with the
             elements in the Table.
V1017 Aql    Elements need confirmation.
V1033 Aql    P var?
V1045 Aql    Min II 13.5.
V1046 Aql    P var? [08321].Min = 2427713.314 + 5.28303d*E [04027].
             Slight reflection effect is possible.
V1064 Aql    Cycles 295d - 410d.
V1072 Aql    sp component of a close pair.
V1075 Aql    d = 0.04P. Min II 13.6.
V1076 Aql    VB A (close preceding).
V1086 Aql    VB. Probably the variable is the sf component.
V1093 Aql    IA type is possible.
V1095 Aql    P var. After JD2429048 - see Table, earlier
             Max = 2427322 + 42.68d*E. Not coloured appreciably.
V1096 Aql    Min II 13.3.
V1097 Aql    Min II 14.0.
V1101 Aql    Possibly UGZ type [03156].
V1113 Aql    The period may be twice shorter.
V1117 Aql    Min II 16.6.
V1125 Aql    Min II 16.0.
V1140 Aql    P var?
V1154 Aql    Min II 14.8; Min II - Min I = 0.70P.
V1165 Aql    According to [04564], constant. In [03932] was not separated
             from a close component which probably led to distortions
             of the light curve.
V1166 Aql    UG type is possible.
V1173 Aql    nf component of a close pair.
V1182 Aql    Min II 8.65.
V1184 Aql    Min II 13.4.
V1200 Aql    VB. The variable is the eastern red component.
V1204 Aql    VB. The variable is the eastern component.
V1208 Aql    A common proper motion star 9.06m in 1' to the south.
V1248 Aql    UG type is possible.
V1251 Aql    Red.
V1261 Aql    Spectral type K2 in HD.
V1269 Aql    VB. The variable is the preceding component.
V1281 Aql    Reddish. SRD type is possible.
V1286 Aql    Possibly the period is accidental.
V1288 Aql    ADS 12182 A (B 12.3m, 36", 287deg).
V1291 Aql    The elements have been determined on the base of magnetic
             field variations. The epoch of minimum intensity of the
             magnetic field is given.
V1295 Aql    Shell star. Dramatic spectral changes were observed [05240].
             The variability is hardly periodic, though P ~100d is
             possible. Sometimes light fluctuations on several days'
             time scale are observed [05880]. IR excess [06277]. For a
             detailed spectroscoric study, with evidence for the
             outflow of matter from the surface, see [04739].
             Considerable magnetic field [04435].
V1297 Aql    d = 0.05P? Min II 14.5.
V1298 Aql    mu alpha = -0.0392s,  mu delta = -1".330.
             The companion of the star BD +4deg 4048 (ro =
             73".8, theta = 151.5 deg).
             One of the absolutely faintest known stars (Mv = +19m).
V1300 Aql    I - K: +5.2, +6.5. Sometimes CO, SiO, OH maser emission.
V1302 Aql    A unique IR object IRC +10420. B - V = +2.7, U - B = +1.9.
             OH, H2O, SiO maser. According to [07437], the energy
             distribution in the IR spectrum (1 - 22mkm) resembles that
             of eta Car. Emissions of neutral metals are observed in
             the spectrum. Increased in brightness during 1925 - 1970;
             Max ~1970.
V1323 Aql    Close VB; var - northern component.
V1325 Aql    VB, np component var.
V1331 Aql    Min II 7.95. According to [04619] P = 1.364076d.
V1333 Aql    Aql X-1. Light variations with P ~1.28d - 1.31d due to
             orbital motion are possible [04625]. Bursts characteristic
             of the XB type are observed [04757]. Lx/Lopt ~500 outside
             nova-like bursts, Lx/Lopt ~5000 during bursts.
V1336 Aql    In 1.6' W from MXB 1916-05. M type is possible.
V1338 Aql    VB. Probably the f component, very bright infrared, is var.
V1340 Aql    d = 0.06P? Intrinsic lightvariations in Max are possible.
V1341 Aql    Min II 13.4. P = 0.3586768D is possible.
V1343 Aql    SS 433. <B - V> = +2.0. Associated with the SNR W 50. Mean
             light varies in the range 14.0 - 14.6 V according to the
             elements Max = 2443662.5 + 165.5d*E [00512]. The depth of
             Min I varies from 0.2m to 0.9m V, the depth of Min II
             varies from 0 to 0.4m V. Two systems of H, HeI, HeII
             emission lines are observed in the spectrum: the
             "stationary" system corresponding to Vr changes from 300
             to 150 km/s with P = 13.1d, and the "relativistic" one,
             corresponding to Vr changes from +50000 to -35000 km/s
             with P = 165.5d. The spectral study [00535]. The system
             apparently consists of an O - B star filling its inner
             Roche lobe and a compact object surrounded by an accretion
             disc wich is precessing with P = 165.5d. Two jets
             consisting of dense condensations of matter emerge from
             the system with relativistic velocity (0.27 c) in opposite
             directions. The luminosity of the disc amounts to not less
             than 60% of the total luminosity of the system [00926, 00953].
             The object may be a former supernova which bursted not
             more than 10**4 years ago.
V1345 Aql    Min II 14.3:, Min II - Min I = 0.46P.
V1349 Aql    Max ~17 pg.
V1352 Aql    VB A (B 14.5m, 6", 175deg).
V1353 Aql    Min II 10.9.
V1355 Aql    Min II 13.3.
V1357 Aql    Possibly P = 1.051d.
V1470 Aql    The variability may be due to the fainter (B) component.
V1472 Aql    SB, Porb = 198d.
V1648 Aql    Brightening over 10 years, probably due to dissipating dust envelope,
             plus quasi-periodic variations.
eta   Aql    P var. P = 7.176344d (JD2373000 - 95100),
             P = 7.176455D (JD2395100 - 2412100). Since JD2412100 -
             see Table. For the whole interval
             Max = 2442794.773 + 7.176735d*E + 2.18d*10**(-8)*E**2
             [08632]. In the UV band the light of a possible A0V
             comparion is apparent.
sig   Aql    ADS 12737 A (B 12.34m, 48", 328deg). Depth of Min II 0.1m.
             In [04627] P = 1.950271d is given according to
             spectroscopic data.
R     Ara    Min II 6.2. VB A (B 8.2mV,  4", 123deg).
S     Ara    (k - b)2 = 0.09. P var [01932, 03126]. Max = 2416284.792 +
             0.45188910d*E (JD2414000 - 19000);Max =
             2419149.797 + 0.45188581d*E (JD2419000 -
             30000) [00752]. Since JD2441000 - see Table. For the
             whole interval, with sufficient accuracy,
             Max = 2420047.2382 + 0.451888176d*E - 1.36d*10**(-10)*E**2
             [03126].
T     Ara    VB A (B 11.0m, 34", 60deg).
X     Ara    Shown in the chart for S5809.
RT    Ara    According to Cannon [01944] who discovered the star's
             variability, a companion 12.0m is present in 0.1m to W
             and somewhat to the north from the variable. Cannon points
             out that at Min light the variable becomes fainter than
             the companion. No sign of the companion's existence was
             found by Hoffmeister [00016] and by Payne-Gaposchkin [00624].
             According to [00624], the mean cycle is ~78d, and RVA
             type is possible.
RW    Ara    d = 0.022P. Min II 8.91. Changes of the shape of the light
             curve due to gaseous streams or a hot spot are possible.
TT    Ara    ZrO bands may be present in the spectrum [03181].
TV    Ara    In the region of the cluster NGC 6208.
TX    Ara    VB A (B 16.5m). Twice shorter period is possible.
XX    Ara    Min II 14.1.
YY    Ara    The star's being an eclipsing or irregular variable is not
             excluded [00424].
AA    Ara    Min II 13.3.
AD    Ara    [A/H] =  -0.4.
AE    Ara    VB A (B 12m, 0.3' sf). P.K. 344-8.1.
             A compast planetary nebula or a symbiotic star. Irregular
             abrupt brightenings by 3m - 4m separated by several years
             are observed [00255]. The spectral data are discussed in
             [08076].
AF    Ara    Min II 13.8.
AW    Ara    Before JD2417300 Max = 2412600 + 186d*E.
BQ    Ara    Double maxima separated by 10d - 20d, with Min II 12.8.
CC    Ara    VB; the variable is nf component.
CH    Ara    Noted on the finding chart for S6062 = V 466 Ara.
CT    Ara    Before JD2420400 Max = 2413080 + 215d:*E;
             since JD2425000 - see Table.
DU    Ara    B - V: +0.52, +0.84. P var. Max = 2418145.560 +
             1.63999d*E (JD2411000 - 21000); Since
             JD2425000 - see Table.
EK    Ara    VB A (B 15m).
EL    Ara    Before JD2420400 Max = 2415140 + 332d*E;
             since JD2425000 - see Table.
ER    Ara    Min II 14.2.
EV    Ara    Before JD2420400 Max = 2413750 + 237d*E;
             since JD2425000 - see Table.
EZ    Ara    P var.
FU    Ara    The depth of Min I is 0.97m and 0.89m,
             the depth of Min II is 0.20m and 0.23m in blue and
             yellow light, respectively.
GK    Ara    Before JD2417800 Max = 2414050 + 237d*E,
             since JD2418400 - see Table.
GM    Ara    Min II 12.8.
HX    Ara    B - V: +0.23, +0.36. A hump on the ascending branch
             (phi = 0.93P) [08118].
KY    Ara    Only one sharp Max (JD2428715 - 712) was observed.
             Possibly a Nova.
KZ    Ara    VB A (B 14.1m sp).
LP    Ara    d = 0.04P? Min II 10.5?
LQ    Ara    In 1959 rapid variations at times for 0.5m near 11m
             were observed; surrounded by a nebula [04001].
LR    Ara    Min II 10.6.
LU    Ara    Min II 10.1?
MQ    Ara    nf component is variable.
MR    Ara    B - V: +0.72, +0.8. [A/H] =  -1.0. P var?
QR    Ara    Shown in the charp for BV 1443.
QU    Ara    VB.
QW    Ara    The variable is np component of the pair.
QX    Ara    Shown in the chart for S5818.
V0340 Ara    B - V: +1.25, +1.68. [A/H] = 0.6.
V0341 Ara    The star is blue; light variations during 4d were not
             accompanied by colour changes. Possibly an eclipsing
             variable [04678].
V0342 Ara    P >= 140d.
V0344 Ara    P >= 170d
V0345 Ara    P >= 180d.
V0349 Ara    Min II 8.8.
V0355 Ara    P > 220d.
V0356 Ara    P > 170d.
V0357 Ara    P >= 220d.
V0360 Ara    Min II 13.8:, Min II - Min I = 0.35P.
V0361 Ara    Min II 13.6:.
V0362 Ara    Min II 15.6:.
V0383 Ara    A star 16.5m is close to the north.
V0421 Ara    Min II 15.1.
V0440 Ara    Min II 14.5:.
V0444 Ara    Min II 14.2.
V0454 Ara    Min II 14.1.
V0480 Ara    Min II 15.5:.
V0484 Ara    RV type is possible (Min = JD2436760).
V0485 Ara    Min II 14.8.
V0489 Ara    Min II 11.9.
V0491 Ara    Min II 11.9.
V0492 Ara    Min II 14.5.
V0494 Ara    RV type is not excluded.
V0501 Ara    Min II 13.8. Shown in the chart for S6114.
V0535 Ara    Min II 7.71. Nonlinear term in the elements:
             -4.4d*10**(-11)*E**2.
V0536 Ara    Min II is present. EB type is possible. P var.
             P = 2.374101d (JD2415000 - 22000); since JD2422000 -
             see Table.
V0539 Ara    VB A (B 9.22m, 12", 269deg). Min II 6.09, d = 0.01P.
             Shown in the chart for BV1441 = V538 Ara.
V0544 Ara    14.5m star sp.
V0609 Ara    Shown in the chart for S5867.
V0610 Ara    EA type is possible.
V0613 Ara    VB (close np companion is NSV10198).
V0616 Ara    Deep Min II.
V0620 Ara    Min II is possibly present.
V0623 Ara    Min II 14.5. Twice shorter period is possible.
V0624 Ara    P >= 220d.
V0625 Ara    P >= 170d.
V0639 Ara    V1 (NGC 6397). Probably not a cluster member.
V0651 Ara    Min II 15.3.
V0653 Ara    Min II 12.6.
V0656 Ara    EW type is not excluded.
V0658 Ara    Min II 16.0.
V0659 Ara    Min II 14.4.
V0668 Ara    Min II 13.8:.
V0675 Ara    P >= 200d.
V0687 Ara    RRC type is possible.
V0700 Ara    Min II 15.7.
V0702 Ara    Min II 14.0.
V0704 Ara    Min II 13.3.
V0705 Ara    Min II 14.4. RR type is possible.
V0716 Ara    Monotonous brightening during JD2436689 - 36838 was
             found. The amplitude is probably greater.
V0722 Ara    Min II 10.3:.
V0728 Ara    Min II 12.8.
V0732 Ara    CEP type is not excluded.
V0743 Ara    RV type is possible.
V0781 Ara    Min II 14.8:.
V0783 Ara    Min II 13.9:.
V0785 Ara    Min II 14.3.
V0787 Ara    RV type is possible. Min JD2436756.
V0789 Ara    Min II 14.8.
V0790 Ara    Min II 14.8.
V0791 Ara    Min II 13.0:.
V0792 Ara    Min II 15.2:.
V0801 Ara    MXB 1636-53. Description of the spectrum [01356].
             Modulation with P ~4h and the amplitude up to 40% was
             found in the broad band optical flux [04944].
V0802 Ara    14.93 - 17.03 B.
V0808 Ara    EW type is possible.
V0820 Ara    Epoch of Min is given. Strong magnetic field. Either an
             eclipsing binary or (more probably) an object similar to
             rotating variables of ACV type.
V0821 Ara    4U 1658-48. Unusua1 X-ray system. Quasiperiodic optical
             variations (P ~20s) with total amplitude 40 percent,
             abrupt bursts on ~20 ms time scale leading to two-fold
             flux increase and light changes by 6m during less than
             two months were observed [04958]. Lx/Lopt = 3.
V0870 Ara    Type DSCT: is also possible.
R     Ari    OH emission.
T     Ari    P var. Max = 2417160 + 313.5d*E (JD2404800 -
             17200); Max = 2434616 + 323.1d*E (JD2419400 -
             34560). Since JD2436560 - see Table. <P> = 319.53d
             (JD2404800 -  44160). Sometimes A < 1.5m.
U     Ari    SiO maser.
V     Ari    Vr =  - 180 km/s.
W     Ari    Maps given in [02544, 06067] are wrong.
X     Ari    B - V: +0.28,  +0.56. P var. Max = 2420785.635 +
             0.6511248d*E (JD2420460 - 33210) [03506]. Since
             JD2433210 - see Table. [Fe/H] = -2.17.
RR    Ari    Min II 6.75:; Min II - Min I = 0.55P. Variability is not
             confirmed by other authors' photoelectric observations.
             V = 5.75.
RS    Ari    Min II 11.0.
RU    Ari    OH emission.
RV    Ari    B - V: +0.29,  +0.44. 0.34P =< M - m =< 0.53P.
             P1 = 0.07195d [08137]; P2 = 0.27554d [07033]. Moments of
             brightest light maxima T = 2435066.400 + 0.31632996d*n
             [02290].
RW    Ari    B - V: +0.35,  +0.46. P var. Max = 2428183.324 +
             0.3543184d*E (JD2428040 - 36700) [03188]. Since
             JD2440900 - see Table. According to [06043] - EA type:
             Min I = 2439384.97 + 3.1754d*E. Total light range
             (11.47 - 13.25 V) [08127] seems doubtful. It is not
             excluded that the eclipses and light increase of RW Ari
             given in [08127] are explained by variability of one of
             comparison stars used.
RX    Ari    d = 0.02P. Depth of Min II 0.10m.
SS    Ari    P var. Min II 10.82:.
ST    Ari    P var. Max = 2427347 + 94.2d*E (1933 - 1939); Max =
             2429525 + 106.6d*E (1939 - 1942); Max = 2430588 +
             95.2d*E (1942 - 1946); Max = 2432118 + 100.0d*E
             (1946 - 1961). Mean elements are given in the Table.
SX    Ari    B - V: -0.10,  -0.12. Epoch of Min is given.
SZ    Ari    d = 0.03P.
TT    Ari    Porb = 0.137551d [08138]. Along with light variations
             typical for Z Cam variables there are sinusoidal variations
             with amplitude of about 0.2m B and variable period:
             P = 0.1329d (1961 - 62), P = 0.1327d (1966) [04931],
             P = 0.1326d (1978) [04935]. Sinusoidal variations are
             superimposed by quasiperiodic oscillations up to 0.2m with
             8 - 20 minutes cycle and irregular flickering up to 0.1m
             in 1 minute.
TU    Ari    P var. Max = 2420463.353 + 0.4716219d*E
             (JD2420463 - 34720). Since JD2436820 - see Table.
TV    Ari    P var.
TX    Ari    P var?
TY    Ari    Form of the light curve varies. Mean value of the period
             is given.
UV    Ari    The second overtone period given in the
             Table is dominating. Sometimes the fundamental
             period P0 = 0.062d and the first overtone period P1 =
             0.047d are observed.
UW    Ari    Amplitude varies. In the interval JD2441581 - 693 - const.
             [07544].
UX    Ari    T = 2440133.766 + 6.43791d*E [06444], where T is epoch of
             conjunction (G5 component is behind K0 component).
             Brightness varies in waves with a period ~Porb, but the
             phase psi of light minimum calculated according to the
             elements given above changes with time: psi = 0.1P
             (1972 - 1974), psi = 0.8P (1976), psi = 0.7P (1977),
             psi = 0.6P (1978). Mean brightness varies, amplitude of
             the wave varies from 0.04m up to 0.15m.
VW    Ari    BDS 1269 A (B 8.33m, 74", 31deg). P2 = 0.089d.
             Metal deficiency. The companion has normal metal abundance.
VY    Ari    SB? Epoch of Min is given.
             Second light variation is also observed: Min =
             2442044.6 + 43.9d*E. A small flare in U band was
             observed.
gam   Ari    VB A (B 4.65m, B 9 V, 7.9", 0deg). Epoch of Min is given.
R     Aur    VB A (B 8.6m, 48", 239deg). P var [07165];
             cycle 64.5a is possible.
S     Aur    P var. In the early fourties of our century the star was
             faint with small and irregular variations.
T     Aur    Min = 2437614.0088 + 0.20437851d*E [08145]. P var?
             <V> = 14.92, <B - V> =  + 0.28. There are light
             fluctuations between the eclipses. Depths of Min are
             0.10m - 0.28m [03195]. Faint nebula with high degree of
             ionization.
U     Aur    H2O maser.
Y     Aur    B - V: +0.70,  +1.06.
Z     Aur    P var [07110]. Max = 2425580 + 110.76d*E
             (JD2416156 - 25580); Max = 2429888 + 113.35d*E
             (JD2425570 - 29900); Max = 2438292 + 135.55d*E
             (JD2429900 - 33300). P = 110d (1965) [03196].
             In 1970 - irregular variations [07338]. <V> =  -165 km/s;
             According to TiO bands the spectrum is M1 [00806].
RS    Aur    P var.
RT    Aur    B - V: +0.39,  +0.80. [A/H] = 0.1. P var. Max =
             2433040.867 + 3.728365d*E (JD2417970 - 33100).
             Since JD2433100 - see Table. Delta(V) var?
RU    Aur    OH emission.
             Mean magnitude probably varies with Pi = 10400d [01059].
RW    Aur    VB A (B 12.5m, dM0e, 1.2", 254deg).
             The companion probably flares with an amplitude
             0.5m - 0.7m [03197, 03198]. Possible period of axial
             rotation is 100d [07067]. OH emission.
RX    Aur    B - V: +0.76,  +1.18; [A/H] =  -0.1, P var?
             Nonlinear term: -0.70d*10**(-6)E**2?
RZ    Aur    P var. Min = 2422616.498 + 3.010593d*E
             (JD2418000 - 26000); since JD2426000 - see Table.
SS    Aur    SB (P = 0.1805939d [06103]).
             Sometimes abnormal behaviour of the star is
             being observed when comparatively numerous and
             small light maxima arise. According to [08151] the
             mean cycle is 51.2d.
SU    Aur    Common proper motion with AB Aur (P = 3'). Associated
             with a small bright nebula. OH emission.
SX    Aur    Min II 8.87. According to [08153] P var:
             Min I = 2418218.7779 + 1.21007653d*E + 0.91d*10**(-10)*E**2.
SY    Aur    B - V: +0.92,  +1.23. [A/H] =  - 0.3. P var [05661].
             Max = 2436853.57 + 10.144330d*E (JD2417900 -
             32380). Since JD2432380 - see Table.
TT    Aur    Min II 9.0.
TV    Aur    S5/6-.
TW    Aur    Mean magnitude varies with P = 1370d.
TZ    Aur    B - V: +0.08,  +0.48. Delta(S) = 2.
UU    Aur    VB A (B 11m, 18", 222deg).
UV    Aur    VB A (B 10.96m, B 9 V, 3.4", 4deg).
             Bright lines [NeIII] and [OIII] in spectrum.
UW    Aur    Epoch of Min is given.
UY    Aur    VB A (B 12m?, 0.8", 212deg). OH emission.
VW    Aur    VB (9.0m, 11.8m, 1.4", 332deg, 1976).
VX    Aur    P var?
WW    Aur    Min II 6.43. Min II - Min I = 0.50P.
XX    Aur    Min II 13.4.
YZ    Aur    B - V: +1.15,  +1.72. [A/H] =  -0.4.
ZZ    Aur    Min II 11.1.
AB    Aur    Common proper motion with AB Aur (P = 3'). Associated
             with a small bright nebula. OH emission. Spectrum
             description [04002].
AE    Aur    Connected with the bright nebula IC
             405. The motion is directed away from Ori OB 1
             association with the velocity 106 km/s.
AG    Aur    According to TiO bands
             the spectrum is M3 [00806].
AH    Aur    Min II 10.70. P var.
AK    Aur    VB B (A = BD +31deg 1370, 8.3m; B 82", 26deg). B - V:
             +0.18.
AM    Aur    Min II 11.0. P var: Min I = 2417617.2 + 13.6182d*E
             (JD2413500 - 19500) [00608]; since JD2425400 - see Table.
AN    Aur    B - V: +1.06,  +1.48. [A/H] =  -0.2.
AO    Aur    B - V: +0.86,  +1.27.
AP    Aur    Min II 11.2. P var: Min I = 2423080.505 + 0.5692965d*E
             (JD2423080 - 35000). Since JD2435000 - see Table.
AQ    Aur    Light curve shape var?
AR    Aur    Min II 6.70. Min II - Min I = 0.50004P. P var: Min I =
             2427887.7217 + 4.13467d*E (JD2427800 - 29500) [04999].
             Since JD2438400 - elements in the Table with an additional
             nonlinear term: -2.2d*10**(-8)*E**2.
AZ    Aur    Close companion 16.3m B.
BC    Aur    Min II 11.7.
BF    Aur    Min II 9.49. P var. Min I = 2434455.3872 +
             1.583217d*E (JD2411760 - 34455) [05038]. Since JD2434455
             - see Table. The two sets of observations are equally well
             represented by the formula: Min I =
             2440628.3643 + 1.5832212d*E + 1.7d*10**(-10)*E**2 [08160].
BH    Aur    P var. Max = 2437352.461 + 0.45608821d*E (JD2417260 -
             42750) [07806]. Since JD2442750 - see Table.
BK    Aur    B - V: +0.86,  +1.26.
CI    Aur    Depth of Min II 0.05m. P var. Min I =
             2439414.573 + 1.869984d*E + 0.020d*10**(-8)*E**2
             (JD2425560 - 42045). Elements given in the Table represent
             observations in the interval JD2439052 - 40654.
CL    Aur    Min II 12.3; Min II - Min I = 0.45P; DII = 0.13P. P var?
             Min I = 2432967.262 + 1.2443666d*E (JD2416900 - 32967)
             [00608]. Since JD2432967 - see Table.
CO    Aur    The first overtone period is
             given in the Table; the second overtone P = 1.4255d.
CQ    Aur    B - V: + 0.86,  + 1.07; Min II 9.14:; Min II - Min I =
             0.52P:; D = 0.096P. P var. Nonlinear term:
              +3.78d*10**(-7)*E**2.
CY    Aur    [A/H] =  -0.3.
DV    Aur    P var. Max = 2426015 + 198.0d*E (JD2426014 - 27400) [00332].
             Since JD2439940 - see Table.
EI    Aur    Min II 15.0.
EM    Aur    Min II 11.7.
EO    Aur    Min II 7.89.
EP    Aur    Min II 10.9. P var?
ER    Aur    [A/H] =  - 1.1. P var? Max = 2432951.54 + 15.69073d*E
             (1949 - 1950) [01059]. In the interval JD2443428 - 874 -
             see Table.
EW    Aur    [A/H] =  - 0.6.
FF    Aur    [A/H] =  - 0.3.
FN    Aur    Min II 12.3. P var?
FP    Aur    d = 0.080P.
FR    Aur    Min II 13.0.
FZ    Aur    d = 0.40d.
GI    Aur    Min II 11.7.
GK    Aur    Min II 14.0; Min II - Min I = 0.62P.
GO    Aur    P var. Max = 2426071 + 292.1d*E (JD2425505 -
             31325); Max = 2432205 + 301.2d*E (JD2432805 -
             36120) [03211]. Since JD2436990 - see Table.
GY    Aur    Min II 13.3.
HL    Aur    Min II 11.0.
HN    Aur    In the cluster NGC 1664.
             Light variations with P2 = 1400d: are
             superimposed by variations with P1 = 165d:.
HP    Aur    Min II 11.28; Min II - Min I = 0.502P. P var. Min I =
             2427445.400 + 1.4228180d*E (JD2427445 - 42683); since
             JD2442712 - see Table.
HR    Aur    Epoch of Min is given.
HS    Aur    Min II 11.2. The value of period given in [02619] must be
             doubled as the system consists of two equal components
             [08164].
HU    Aur    Min II 12.4.
HW    Aur    Min II 12.6.
HZ    Aur    Sometimes short period variations of Vr with the amplitude
             3 km/s and of brightness in U with the amplitude 0.02m are
             also observed. Max Vr = 2439454.900 + 0.073502d*E
             [05259]. P (DeltaU) = 0.07396d [04818].
II    Aur    Min II 15.0:.
IM    Aur    Min II 8.05:.
IQ    Aur    Epoch of Min is given.
IS    Aur    VB. The range of combined brightness variation is given.
             It is not known which of the components varies.
IU    Aur    P var. There is an additional periodic term in the elements:
             -0.00627d*sin (2.221deg*E + 15deg). The ratio of Min II
             depth to Min I depth is 0.78. There is secular deepening
             of both minima. The depth of Min I increases by 0.016m per
             year. The range of light variation in the Table is given
             for 1979.0 (Min II 8.69). Orbital inclination is increasing
             by 0.5deg per year [05181] due to orbital precession caused
             by a third body. Spectrum description [08166].
KO    Aur    Min II 11.2.
KR    Aur    <B - V> =  +0.10, <U - B> =  -0.95. SB (P = 0.1628d [09045]).
             Spectrum description [08169, 08170]. Wide hydrogen emission
             lines. Long maxima and minima lasting for years are
             superimposed by rapid light variations by 1 - 2m in
             several days or fortnights and by 0.5m in dozens of
             seconds [08168, 08170]. The source of soft X-rays [05191].
KS    Aur    VB A (12.5m, 5", 94deg).
KV    Aur    Flat waves with a cycle about 750d are sometimes
             superimposed by comparatively rapid fluctuations.
KW    Aur    VB A (B 11.0m, 11.1", 352deg, 1909; C 7.99m, 14.5",
             226deg, 1923); SB1 (P = 3.788568d). Mean light level
             varies synchronously with orbital motion. Besides main
             pulsational period there are two more periods of nonradial
             pulsation: P1 = 0.096533d, P2 = 0.088243d.
KX    Aur    In the IC 405 nebula.
KY    Aur    In the IC 405 nebula.
LY    Aur    VB A (B 9.1m, 0.6", 249deg, 1958). Min II 7.26; d = 0.017P.
MR    Aur    Min II 15.5.
MT    Aur    d = 0.02P.
NP    Aur    P var. Since JD2437720 - see Table.
NU    Aur    Blazhko effect. Pi = 179d:.
NV    Aur    OH, SiO, H2O maser.
NW    Aur    In the region of the NGC 1893. Min II 14.7.
             According to [07160] no minimum was recorded during
             visual observations covering twice all phases.
NX    Aur    In the cluster NGC 1893.
OP    Aur    In the cluster Stock 8.
OX    Aur    VB A (B 10.0m, 22.4", 224deg). P1 = 0.115442d.
             Mean brightness probably varies.
PR    Aur    The chart in [07806] is wrong.
PY    Aur    Possibly a cepheid.
QR    Aur    Epoch of Min is given.
QY    Aur    SB.
V0348 Aur    VB A (B 13.43m, 24", 44deg).
V0353 Aur    During several decades the star brightened by 0.06m in a
             year. Possibly a planetary nebula in the process of
             formation.
V0358 Aur    In the region of the cluster NGC 2099.
V0411 Aur    The HD catalogue identifies HD 32447 with BD+30 775, wich
             is V0411 Aur. In the HDE Atlas V0411 Aur = HD 282867, and
             HD 32447 is a different star.
V0431 Aur    P = 16.86d detected in HIPPARCOS data.
V0433 Aur    SB?
V0527 Aur    Also might be a low-amplitude Cepheid.
bet   Aur    VB A (B 14.1m, 13", 174deg). Min II 1.98.
eps   Aur    VB A (B 14.0m, 21", 224deg). d = 0.037P.
             Survey of the physical properties of the system [02041,
             02042, 03070, 03216, 03217, 08174]. The spectrum probably
             varies even outside eclipses. The eclipses are probably
             due to a disk of gas and dust surrounding the hot
             companion. The brightness has physical fluctuations
             with the amplitude up to 0.24m and the cycle about 110d
             [02040] which hinder revealing the possible Min II.
             Similar cycle was discovered also in the fluctuations
             of Vr.
zet   Aur    Range of light variation strongly depends on lambda:
             4.98 - 5.53 B, 5.36 - 7.33 U. d = 0.039P var:
             37.58d <= d <= 38.07d [05486]. Light fluctuations of
             K star by 0.05m [05539].
tet   Aur    VB A (B 7.5m, 2", 8, 331deg, 1924).
             According to [04034] the period of magnetic field variation
             is 3.618d.
U     Boo    Delta(m) var (from 0.9m to 2.4m).
V     Boo    P var. Amplitude strongly varies.
W     Boo    According to [06994], P = 30d +-.
Z     Boo    H2O maser.
RS    Boo    Delta(S) = 2. P var. Before JD2435000 Max =
             2418115.5867 + 0.37733691d*E; since JD2435000 - see
             Table. Changes of the height of maxima: Max (minimal
             height) = JD2442500 + 533d*E; a shorter cycle of changes
             is possible: P ~ 58 - 62d [04832].
RU    Boo    B - V: +0.09, +0.44.
RX    Boo    H2O, SiO, OH maser.
SS    Boo    Depth of Min II 0.1m.
ST    Boo    P var. Max = 2439236.032 + 0.6222968d*E (1966 - 1974).
             Mean elements 1911 - 1974 - see Table. Blazhko effect: Min
             (O - C) = 2442203 + 284d*n. Delta(S) = 11.
SU    Boo    D = 0.032P. Min II 12.04. P var.
SV    Boo    B - V: +0.17,  +0.44. P var?
SW    Boo    B - V: +0.09,  +0.39. P var. Before JD2426500
             Max = 2421840.295 + 0.5134948d*E [02008, 02011]. Since
             1960 - see Table. Secondary oscillation: Max (height of
             Max) = 2441037.33 + 12.997d*E. According to [04833], the
             magnitude in Max varies between 10.5 and 11.6 V.
SZ    Boo    P var?
TU    Boo    Min II 12.4.
TV    Boo    B - V: +0.10,  +0.22. [Fe/H] = -2.42.
             Blazhko effect, Pi = 16.14d [07116].
TW    Boo    B - V: +0.11,  +0.40. Delta(S) = 12. P var. Before
             JD2426890 Max = 2420340.551 + 0.53227557d*E;
             since JD2426890 - see Table.
TY    Boo    Min II 11.35.P var.
TZ    Boo    Min II 10.82 (var). dII = 0.09P. P var. Depths of minima
             vary from 10.8 to 11.0 V with P ~3.5 yrs; sometimes Min II
             is deeper than Min I. Some other parameters of the shape
             of light curve are also variable. In ~1960 the period
             changed abruptly; other period variations were also noted.
UU    Boo    B - V: +0.03,  +0.44. P var. Period change ~JD2432700
             [03230]. Earlier Max = 2424967.310 + 0.45690626d*E [03229].
UW    Boo    Min II 10.5.
UX    Boo    According to [02136], Delta(m) ~0.5m pg, EW?
UY    Boo    Delta(S) = 12.6. P, Delta(m) var. Before JD2425500
             Max = 2411459.819 + 0.6508552d*E; Max =
             2425688.836 + 0.6507849d*E (JD2425500 - 28670) [01702];
             Max = 2432306.759 + 0.650799d*E (JD2428670 - 32300)
             [02431]. Since JD2435900 - see Table.
VW    Boo    Min II 10.93. P var. Nonlinear term:
             -0.084d*10**(-9)*(E - 7500)**2.
WY    Boo    Possibly P = 90d.
XY    Boo    Min II 10.61. P var.
YZ    Boo    Delta(S) = 0. Delta(m) var, the shape of the light curve
             varies [08186].
ZZ    Boo    Min II 7.44. Possible radio source.
AC    Boo    Min II 10.55. P var? Depth of minima and level of maxima
             are variable.
AD    Boo    Min II 9.9.
AE    Boo    P var. (k - b)2 = 0.01.
AG    Boo    Blazhko effect is possible.
AK    Boo    Min II 16.3.
AO    Boo    P var. Mean period is given.
AR    Boo    Min II 14.5. P var.
AS    Boo    Blazhko effect is possible.
BD    Boo    Blazhko effect is possible.
BE    Boo    Scatter in the light curve near max light;
             P var? [05264]. The value of the period in the
             Table may be spurious.
BG    Boo    Min II 14.3.
BI    Boo    In the region of the globular cluster NGC 5466.
BK    Boo    Min II 15.3.
BL    Boo    V 19 (NGC 5466). B - V: +0.12,  +0.25. [Fe/H] = -1.35.
             "Anomalous cepheid". Radial velocity cluster member.
BN    Boo    In the region of the cluster NGC 5466.
BO    Boo    The shape of the light curve varies: magnitude in
             Max - from 14.5 to 15.0.
BP    Boo    5.51 V.
BR    Boo    The mean light curve shows scatter which may evidence for
             the necessity to improve the period.
BU    Boo    P var. Mean period is given. AO Boo. The mean light curve
             could not be obtained.
BW    Boo    Min II 7.17. Min II - Min I = 0.450P. DII = 0.06P. SB1.
BX    Boo    VB A (B 10.6m, 36", 156deg). P var. According to other
             sources: Min = 244076730 + 0.741285d*E [07955];
             Min = 2440767.26 + 0.6080722d*E [05054].
CC    Boo    The star is not red.
CD    Boo    The star is not red.
CK    Boo    Min II 9.23.
CP    Boo    P > 0.125d.
EL    Boo    Type E: is also possible.
gam   Boo    VB A (B 12.5m, 33", 111deg, 1925). Delta(m) var. Radial
             velocity varies with P = 0.25d +-0.02d [04914].
kap 2 Boo    ADS 9173 A (B = kappa1 Boo, 6.69m, SB, F2V, 13",236deg).
             According to [07015], P = 0.0668d.
             Beat period ~16d [06086, 07015].
ksi   Boo    ADS 9413 AB (4.7m, G8V; 6.6m, K4V; A = 4.884", P = 149.95a).
             LiI lambda 6708 line is present in the G8V spectrum. Both
             spectra show manifestations of chromospheric activity,
             emissions of H and K Ca II. Soft X-ray source. Probably it
             is component A that is variable, though variability of H
             and K CaII emission with the cycle 10 - 11 years
             is observed for component B.
i     Boo    ADS 9494 B (A 5.1m, G0; a = 3.8", e = 0.43, P =
             225a). Min II 6.29. P var. Min = 2434132.517 +
             0.267812271d*E + 0.115242d*10**(-9)*E**2 (1916 -
             1958) [03239]; Min = 2438513.4166 + 0.2678143d*E
             (1947 - 1967) [08191]; since 1968 - see Table. Detailed
             studies of period changes [05222, 07352, 07353, 08181]. Sudden
             period changes at JD2423800, 29300, 32300, 35150 are
             possible. The shape of the light curve and the depth of
             Min II are also variable. According to [02020], it is also
             possible that ADS 9494 A is variable, with the amplitude
             up to 0.09m.
S     Cae    <B - V> =  +0.33. P < 1d.
X     Cae    (k - b)2 = 0.22.
RX    Cae    Variability type and spectral type (F3/F5II) do not agree.
R     Cam    S2/5:e. P var.
T     Cam    S5/5e.
U     Cam    Interfering P1 = 435.45d, P2 = 223.17d; P3 = 3000d [01053].
V     Cam    H2O, SiO maser.
Y     Cam    EA/SD. SB1. Min II 10.60. P var. Min =
             2424434.5071 + 3.3054975d*E + 0.1215d*
             sin (0.0543deg*E + 186.8deg) (JD2411400 - 33300) [00978];
             Min = 2437375.4923 + 3.3055069d*E + 5.3d*10**(-8)*E**2
             (JD2437375 - 41000) [07166]; since JD2440000 - see Table.
             The primary component is a DSCTC variable [07166] with
             A <= 0.05m B. According to [04192], the pulsational period
             is possibly synchronized with the orbital motion and
             remains practically constant (0.066458d) during a long time
             interval.
Z     Cam    SB2. Lower conjunction of the G component
             T = 2438470.841 + 0.289840d*E [05365]. Outside outbursts
             the light curve is modulated with spectroscopic elements
             and has a shoulder at the phase 0.88P and a broad, shallow
             dip at the phase 0.15P. Outside maxima flickering up to
             0.5m with P ~ 16s - 18s is observed. During maxima
             brightness fluctuations are small [05365, 04193].
RS    Cam    Mean brightness varies.
RU    Cam    [A/H] =  +0.9:. P var. Min = 2417610.1 + 22.187d*E (1908 -
             1917), Min = 2421315.3 + 22.121d*E (1917 - 1922),
             Min = 2423195.6 + 22.217d*E (1922 - 1931), Min =
             2426350.4 + 22.138d*E (1931 - 1951), Min =
             2433700.2  + 22.162d*E (1951 - 1961), Min =
             2437356.9 + 22.055d*E (1961 - 1965) [03243].
             Unusual variable. The shape of the light curve varies.
             Before 1964 broad maxima and sharp minima were observed;
             Delta(m) varied by the factor  of 2, with a possible cycle
             5.1a [03241]. After 1964 - 1966 Delta(m) decreased abruptly
             (to 0.4m - 0.1m and smaller), the light curve became
             symmetric; the mean light varies in the range of 0.3m B.
             The period varies irregularly in the interval
             19.4d - 23.5d. Groups of oscillations are observed to
             replace  one another, with phase shifts up to 0.5p [04206].
             Unusual spectrum with intense CN and weak C2 bands.
RW    Cam    [A/H] =  +0.4. P var?
RX    Cam    B - V: +1.05,  +1.48. [A/H] = 0.
RY    Cam    Possibly P2 = 150.8d.
SS    Cam    d = 0.06P. Min II 10.35:. P var; nonlinear term:
             +2.04d*10**(-9)*E**2.
SV    Cam    Depth of Min II 0.15m: pg. P var. A cycle of 50a may be
             present in period changes. The elements in the Table are
             valid since 1967.5.
SW    Cam    P var. Before JD2437600 Max = 2434448 + 254.2d*E. Since
             JD2440000 - see Table.
SZ    Cam    Member of the open cluster NGC 1502. ADS 2984 B (A = NSV
             1458 7.1m V; B 18", 304deg). Min II 7.24, D II = 0.17P.
             P var. Since 1970 - see Table; earlier
             Min I = 2427533.5191 + 2.6984166d*E [02071].
TU    Cam    Min II 5.22.
TV    Cam    [A/H] = -0.2.
TX    Cam    SiO maser.
UY    Cam    Delta(m) var (0.2m - 0.5m V) [03528].
UZ    Cam    P var? Before JD2428700 Max = 2427992 + 231.0d*E [00114];
             since JD2440000 - see Table.
WW    Cam    d = 0.013d. Min II 11.1.
XX    Cam    During 1898 - 1980 a single symmetric Min JD2429632 was
             observed which lasted for 94d. Brightness fluctuations up
             to 0.2m during several dozens of minutes  [04271]. Hydrogen
             deficiency and carbon excess in the spectrum. Some authors
             express doubt about the star's being an RCB variable; in
             particular, they note the lack of IR excess [05423, 05430].
AB    Cam    [A/H] = -0.1.
AD    Cam    [A/H] = -1.0.
AE    Cam    Min II 15.8.
AH    Cam    VB A (B 7"). P var. Max = 2433897.519 +
             0.3687404d*E (JD2427000 - 33897) [02305]. Since
             JD2438000 - see Table. Magnitude in Max varies with a
             possible cycle Pi = 46 P [03506].
AK    Cam    P var. Min = 2426393.180 + 2.226780d*E (JD2426390 - 36610)
             [02594]; since JD2436000 - see Table.
AS    Cam    d = 0.009P. Min II 8.97, DII = 0.06P, Min II - Min I =
             0.437P.
AT    Cam    Min II 10.6.
AU    Cam    Very red.
AV    Cam    d = 0.04P.
AW    Cam    Min II 8.36.
AX    Cam    Detailed spectral studies [07191], [07192].
AY    Cam    Min II 10.23, DII = 0.12P, dII = 0.02P. According to
             [03260], the spectrum is A5.
AZ    Cam    Min II 10.8.
BI    Cam    Delta(m) = 0.9m pg.
BK    Cam    During 1912 - 1932 periodic (P ~4.4a) spectral changes
             were observed which came to an end by 1937 [04282].
BM    Cam    SB1 (P = 80.174469d; e = 0.35). Epoch of Min light is given.
CZ    Cam    P = 267.79d, semiregular behavior unusual for B5 stars.
R     Cnc    SiO maser.
S     Cnc    In the field of Praesere (NGC 2632) cluster. d = 0.015P.
             Min II 8.39. P var.
U     Cnc    VB A (B 3"). In the field of Praesepe (NGC 2632) cluster.
V     Cnc    S0.5/6e. ADS 6763 A (B 13.5m, 10", 270deg).
RS    Cnc    P2 = 1700d. Tc lines are present in the spectrum.
RT    Cnc    P2 ~600d.
RU    Cnc    d = 0.035P. Min II 10.21:, DII <= 0.07P.
RW    Cnc    P var. Since JD2437000 - see Table. According to [02088],
             Max = 2421339.380 + 0.5471932d*E +
             0.57d*10**(-9)*(E - 5800)**2 + 0.028d*cos0.0215deg*
             (E + 2260) + f(psi, hi); here the last term is the sum of
             two short period oscillations and is given in graphical
             form, since the main period (0.547d) varies with
             Pi1 = 29.9d and Pi2 = 91.1d. Magnitude in Max varies from
             10.7m to 11.8m, in Min from 12.3m to 12.6m.
RY    Cnc    In the region of the open cluster NGC 2632 (Praesepe),
             non-member. B - V: +0.58, +1.05. P var. Before JD2436000
             Min = 2429334.445 + 1.0929500d*E; since
             JD2436000 - see Table.
RZ    Cnc    Min II 9.21. d = 0.015P:. Ellipsoidal components.
SS    Cnc    Delta(S) = 1.2. P var?
SV    Cnc    B - V: +0.10, +0.52.
SY    Cnc    Flickering with P ~20s - 34s [05959]. Spectral investigation
             [04286].
TT    Cnc    (k - b)2 = 0.11. P var. Before JD2430700
             Max = JD2425647.452 + 0.5634445d*E [03506].
             Since JD2439800 - see Table. Blazhko effect, Pi = 89d
             [05271].
TW    Cnc    d = 0.014P. Depth of Min II 0.1m pg.
TX    Cnc    Member of the open cluster Praesepe (NGC 2632). Min II
             10.32.
TY    Cnc    d = 0.013P. P var.
UU    Cnc    Min II 9.2, JD (Min II) 2435608.5. SB1. The light curve is
             unstable. Spectral studies [01881], [03149], [04289].
UV    Cnc    In the region of the Praesepe (NGC 2632) cluster.
UZ    Cnc    Min II 11.4.
VY    Cnc    Min II 12.3:.
VZ    Cnc    (k - b)2 = 0.32. Beat phenomenon for two oscillations is
             observed. According to [02125], for the middle of
             the ascending branch T (<m>)  = 2433631.84615 +
             0.17836376d*E + 0.00193d*sin(2*pi*psi(<m>) -
             0.00371d*cos*2*pi*psi(<m>); here the phase of the beat
             period psi(<m>) is computed with the elements T(<m>) =
             Spectral investigation [02126].
WW    Cnc    According to [07531], the period does not vary since 1933.
             A number of minima by
             BBSAG contradict the tabulated elements.
WX    Cnc    Min II 10.7.
WY    Cnc    VB A (B 12.8m,  -20", 0deg). Min II 9.60.
XX    Cnc    In the region of the Praesepe (NGC 2632) cluster.
XZ    Cnc    Min II 10.2.
YY    Cnc    According to [03263], the star is probably an irregular
             variable.
YZ    Cnc    Oscillations with P = 133.2m are observed in maximum light
             [06249].
ZZ    Cnc    d = 0.02P:.
AC    Cnc    Min II 14.7. <Max> = 14.5.
             The brightness outsibe eclipses varies in the range 13.8 -
             15.2B. 3 deep minima contradict the tabulated
             elements [04460]. The identification with the X-ray
             source H 0857+13 is not excluded.
AD    Cnc    Min II 13.4.
AH    Cnc    Member of the open cluster M 67 (NGC 2682). Min II 13.68.
             Nonlinear term: +1.56d*10**(-10)*E**2.
             Cyclic period variations (with different cycles) are also
             possible [04475].
AO    Cnc    Min II 13.4.
AP    Cnc    P var?
AU    Cnc    Possible member of the cluster praesepe (NGC 2632).
AV    Cnc    Possible member of the cluster Praesepe (NGC 2632).
AW    Cnc    Possible member of the cluster Praesepe (NGC 2632).
AX    Cnc    Possible member of the cluster Praesepe (NGC 2632).
AY    Cnc    Possible member of the cluster Praesepe (NGC 2632).
AZ    Cnc    Possible member of the cluster Praesepe (NGC 2632).
BB    Cnc    Delta(mu) > 6.0. Possible member of the cluster
             Praesepe (NGC 2632).
BC    Cnc    Delta(mu) > 4.0. Possible member of the cluster
             Praesepe (NGC 2632).
BD    Cnc    Possible member of the cluster Praesepe (NGC 2632).
BE    Cnc    Possible member of the cluster Praesepe (NGC 2632).
BG    Cnc    Possible member of the cluster Praesepe (NGC 2632).
BH    Cnc    Possible member of the cluster Praesepe (NGC 2632).
BI    Cnc    The elements were determined by Winzer. Epoch of Max
             in U band is given.
BK    Cnc    Possible member of the cluster Praesepe (NGC 2632).
BM    Cnc    SB (P = 585.4154d [06568]). The elements in the Table
             represent the moments of maximal (B - V).
BN    Cnc    Member of the cluster Praesepe (NGC 2632).
BQ    Cnc    SB.Member of the cluster Praesepe (NGC 2632).
BR    Cnc    VB A (B 14.2m, 30", 268deg). Member of the cluster
             Praesepe (NGC 2632).
BS    Cnc    Member of the cluster Praesepe (NGC 2632).
BT    Cnc    Member of the cluster Praesepe (NGC 2632).
             Oscillations with other periods are superimposed.
BU    Cnc    Member of the cluster Praesepe (NGC 2632). According to
             [04483], P = 0.071d is not confirmed; during different
             nights P = 0.0534d, P = 0.059d and several other
             periodicities were observed.
BV    Cnc    Member of the cluster Praesepe (NGC 2632).
BW    Cnc    Member of the cluster Praesepe (NGC 2632).
BX    Cnc    Member of the cluster Praesepe (NGC 2632).
BY    Cnc    Member of the cluster Praesepe (NGC 2632).
BZ    Cnc    In the region of the Praesepe (NGC 2632) cluster.
CC    Cnc    Cycle <= 90d.
CD    Cnc    Possible member of the cluster Praesepe (NGC 2632).
CE    Cnc    In the region of the Praesepe (NGC 2632) cluster.
CF    Cnc    In the region of the Praesepe (NGC 2632) cluster.
CG    Cnc    In the region of the Praesepe (NGC 2632) cluster.
CH    Cnc    In the region of the Praesepe (NGC 2632) cluster.
CI    Cnc    Possible member of the cluster Praesepe (NGC 2632).
CK    Cnc    In the region of the Praesepe (NGC 2632) cluster.
CL    Cnc    In the region of the Praesepe (NGC 2632) cluster.
CM    Cnc    Possible member of the cluster Praesepe (NGC 2632).
CN    Cnc    Possible member of the cluster Praesepe (NGC 2632).
CO    Cnc    In the region of the Praesepe (NGC 2632) cluster.
CP    Cnc    In the region of the Praesepe (NGC 2632) cluster.
CR    Cnc    In the region of the Praesepe (NGC 2632) cluster.
CS    Cnc    In the region of the Praesepe (NGC 2632) cluster.
CU    Cnc    G 9-8 = G 40-25. VB A (B = CV Cnc, 13", 347deg),
             common mu. In the region of Praesepe (NGC 2632) cluster,
             non-member.
CV    Cnc    G 40-26. VB B (A = CU Cnc).
CY    Cnc    Member of the cluster Praesepe (NGC 2632).
CZ    Cnc    Equinox in [08354] must be 2000.0.
DD    Cnc    In the region of the Praesepe (NGC 2632) cluster.
DF    Cnc    In the region of the Praesepe (NGC 2632) cluster.
             Posibly non-member.
DG    Cnc    In the region of the Praesepe (NGC 2632) cluster.
             Possibly non-member.
DH    Cnc    Possible member of the cluster Praesepe (NGC 2632).
DI    Cnc    Possible member of the cluster Praesepe (NGC 2632).
DL    Cnc    VB. In the region of the Praesepe (NGC 2632) cluster.
DM    Cnc    Possible member of the cluster Praesepe (NGC 2632).
DN    Cnc    In the region of the Praesepe (NGC 2632) cluster.
DO    Cnc    In the region of the Praesepe (NGC 2632) cluster.
DP    Cnc    In the region of the Praesepe (NGC 2632) cluster.
DQ    Cnc    In the region of the Praesepe (NGC 2632) cluster.
             Possibly non-member.
DR    Cnc    In the region of the Praesepe (NGC 2632) cluster.
DS    Cnc    In the regiom of the Praesepe (NGC 2632) cluster.
             Possibly non-member.
DT    Cnc    In the region of the Praesepe (NGC 2632) cluster.
DU    Cnc    In the region of the Praesepe (NGC 2632) cluster.
FV    Cnc    The type is doubtful.
kap   Cnc    SB (P = 6.39316d). In [04487] the light variability was not
             confirmed.
R     CVn    P var. Max = 2411768 + 325.4d*E (JD2411730 - 26430) [01701];
             Max = 2432074 + 332.8d*E
             (JD2426750 - 32100); since JD2432100 - see Table.
T     CVn    SRA? Delta(m) strongly varies.
U     CVn    OH, H2O emission.
V     CVn    H2O, SiO maser.
W     CVn    B - V: +0.15, +0.42. P var.
             Nonlinear term: -368*10**(-13)*E**2. Delta(S) = 7.
Y     CVn    P2 = 2000d.
Z     CVn    B - V: +0.20, +0.33. P var. Max = 2413000.262 +
             0.6538236d*E (JD2413000 - 23170); Max =
             2423860.355 + 0.6539052d*E (JD2423860 -
             31800) [01702]; Max = 2432943.645 + 0.653824d*E
             (JD2431800 - 40200) [06457]. Since JD2438900 - see Table.
             Blazhko effect: Min. ampl. = 2439176.12 + 22.75d*E [03267].
             Amplitude varies by 0.5m B, extremal periodic deviations
             of the epoch of Max from linear elements are  +-0.02d.
             Delta(S) = 8.
RR    CVn    B - V: +0.09, +0.45. [Fe/H] = -1.33.
             The light curve shape and Delta(m) var.
RS    CVn    Min II 8.19; Min II - Min I = 0.506P; d = 0.033P.
             P var. Nonlinear term: -1.00d*10**(-8)*E**2. Wave-like
             distorsion with the amplitude from 0.09m up to 0.20m and
             with the period 4.7917d close to the orbital one is
             observed on the light curve out of eclipses [07209].
             The wave is migrating on phase in the direction of phase
             decreasing with a migration period of 9.48 years [05800].
RU    CVn    B - V: +0.10, +0.39. P var. Max = 2420227.338 +
             0.5732502d*E (JD2418801 - 29436) [05436]; Max =
             2420227.398 + 0.57324647d*E (JD2418979 -
             36665) [03271]; since JD2434483 - see Table.
RV    CVn    V141 (M3/NGC 5272). Not a member of the cluster.
             Min II 15.81.
RX    CVn    B - V: +0.17, +0.41. P var?
RZ    CVn    B - V: +0.12, +0.43. P var. Max = 2424621.489 +
             0.56740036d*E (JD2424620 - 31000) [00188];
             Max = 2437823.433 + 0.5674174d*E (JD2434470 -
             37830); since JD2438200 - see Table.
ST    CVn    P var? Delta(S) = 4.8.
SV    CVn    P var. Max = 2427434.911 + 0.66805653d*E
             (JD2426000 - 32000) [00752]; since JD2439500 - see Table.
SW    CVn    P var. Max = 2431139.791 + 0.44164922d*E
             (JD2425640 - 32000) [00752]; since JD2436200 - see Table.
TX    CVn    SB2 (P = 70.8d) [04504].
UU    CVn    In the region of the globular cluster NGC 5466. P var.
             Max = 2437817.312 + 0.5409589d*E (JD2436360 - 39945);
             since JD2439945 - see Table.
UV    CVn    In the region of globular cluster NGC 5466, non-member.
             P var. Max = 2419446.156 + 0.6316090d*E (JD2419440 - 34455);
             since JD2434450 - see Table.
UW    CVn    In the region of the globular cluster NGC 5466.
UX    CVn    Min II 11.94. U - B: -1.05, -0.99; B - V: -0.29, -0.23.
VV    CVn    Min II 14.3:.
VW    CVn    Min II 12.4. P var. Min I = 2435923.246 + 0.8499757d*E
             (JD2427900 - 36000); since JD2435900 - see Table. The
             variable is not marked on the map. It is by 6mm to the
             west and 3mm to the north of the comparison star C.
VZ    CVn    Min II 9.54.
WW    CVn    Blazhko effect is possible.
WY    CVn    V 205 (M3/NGC 5272). Member of the cluster? Blazhko effect
             is possible.
WZ    CVn    V 206 (M3/NGC 5272). Non-member? Blazhko effect.
XX    CVn    In the region of M3 (NGC 5272) globular cluster. Member
             of the cluster?
YZ    CVn    d = 0.055P, depth of Min II 0.05m vis.
AA    CVn    [Fe/H] = -1.78.
AD    CVn    [Fe/H] = -1.39.
AF    CVn    [Fe/H] = -1.19.
AG    CVn    [Fe/H] = -2.01.
AH    CVn    [Fe/H] = -2.01.
AI    CVn    Radial multiperiod pulsations: P0 = 0.2085d,
             P1 = 0.1529d, P2 = 0.1259d, P3 = 0.1158d.
AK    CVn    [Fe/H] = -1.19.
AM    CVn    The light curve is a double wave. Min II sometimes
             disappears. The depth of Min I changes also. Epoch of
             Min I is given in the Table. P var; dP/dt = +0.012s per
             year. Elements for 1978 are given in the Table. The
             brightness fluctuates with the cycle of 115 - 120s,
             sometimes the periodicity with P = 26.3s is observed.
             Probably it is a close binary semidetached system of two
             white dwarfs with an accretion disk and a hot spot.
AN    CVn    [Fe/H] = -1.54.
AQ    CVn    Similar to horizontal branch stars in globular clusters.
             A flare lasting 20 minutes was observed.
BF    CVn    G 123-75 = G 164-32. VB A (B = G 164-31, 13.16m,
             dM3.5e; 17", 225deg). Flares in the combined light of the
             system (Delta(U) up to 0.95m) were observed.
BG    CVn    P1 = 1186s, P2 = 780s.
BH    CVn    SB. Reflection effect Delta(m) = 0.013V.
BI    CVn    Min II 10.70. P var?
CS    CVn    HIPPARCOS data contradict the luminosity class V.
alf 2 CVn
             VB A (B 5.60m, F0V, 19.6", 228deg).
             Epoch of Min is given.
R     CMa    Min II 5.78. P var [03280, 06314].
             The star shows anomalies of the light curve [03281, 03282].
V     CMa    VB B (A = CPD -31deg 1311, 9.4 m; B 16", 90deg).
Z     CMa    Strong IR excess. Shell spectrum. Several lines show P Cyg
             profiles. The star is located in a nebula rich in details.
             A bright wisp of nebulosity near the star  has continuons
             spectrum, probably identical to that of the star [04002].
RR    CMa    Min II 13.1.
RT    CMa    Min II 11.5.
             P = 1.293745d is possible taking into account the epoch
             from [03283].
RX    CMa    d = 0.027P. Min II 11.1. P var. During JD2441700 - 43000
             - see Table.
RZ    CMa    P var? Since JD2435500 - see Table.
SW    CMa    Min II 9.9. Min II = JD2426709.366; Min II - Min I =
             0.316P.
SX    CMa    Min II 10.3.
TU    CMa    Min II 10.1.
UW    CMa    Min II 5.25. Gaseous streams, expanding gaseous envelope.
             Minima are asymmetric; other peculiarities of the light
             are observed. A number of spectral lines have P Cyg
             profiles.
             The line profiles are observed to vary with the phase of
             the orbital period, and also ([07227], according to Sanyal)
             with characteristic time <1h.
UX    CMa    Min II 12.3.
VW    CMa    Min II 9.1.
VY    CMa    ADS 6033 A (B 9.2m, 0.5", 168deg; C 11.5m, 2.7", 291deg,
             D 11m, 2.9", 347deg, ...). H2O, OH, SiO maser.
             B - V:  +2.3.
             In the region of the
             young open cluster NGC 2362. Embedded in a
             reflecting nebula. The companions may be details
             of the nebula; some of them are probably variable [02159,
             03287]. Surrounded by an envelope of gas and dust or a disk
             of 0.45" (lambda = 5 mkm) angular size. Secular decrease
             of brightness since 1801. Cyclic variations of brightness
             with Delta(m) from several tenths of a magnitude to 3m on
             time scale from 200d to 1900d. TiO and ScO emission bands
             in the spectrum. Spectroscopic studies [03287, 05282, 06133].
WW    CMa    RR, Max = 2428570.09 + 0.499355d*E [00613]. CEP,
             Max = 2428146.6 + 5.7660d*E [00514]. These systems of
             elements are contradicted by 94 photographic observations
             (Erleksova) and 12 photoelectric observations (Irwin,
             [03288]).
XY    CMa    d = 0.04P:.
ZZ    CMa    Min II 13.0.
AE    CMa    d = 0.02P:.
AN    CMa    d = 0.02P:.
AO    CMa    In the field of the open cluster Ruprecht 18.
AR    CMa    d = 0.025P:.
AS    CMa    d = 0.04P.
BN    CMa    Min II 14.9.
BQ    CMa    In the region of the open cluster NGC 2354.
BS    CMa    Min II 14.5.
CC    CMa    Mean brightness varies?
CE    CMa    Min II 13.3. Min II - Min I = 0.663P.
CH    CMa    Min II 12.9.
CK    CMa    Min II 15.4.
CM    CMa    Min II 13.1.
CO    CMa    Mean brightness probably varies with P ~700d.
CR    CMa    Min II 12.4.
CV    CMa    Min II 13.5. DII = 0.09P. Min II - Min I = 0.358P.
CW    CMa    Min II 8.94. SB2.
CX    CMa    Min II 10.3.
DD    CMa    Min II 11.8.
DE    CMa    Min II 13.4.
DS    CMa    VB A (B 15.8m, 10", 130deg).
DV    CMa    JD2425300 - 27500: P - see Table; since JD2428000 P ~400d.
EF    CMa    d = 0.02P.
EW    CMa    VB Delta(m) <= 0.5m, 0.102", 112.1deg, 1952.203).
             SB (P = 0.261975d). Brightness variations are not related
             to the orbital phase. Shell star (probably an extended
             atmosphere of one of the components and the common shell
             around the system). Spectral studies [4592 - 4596].
EX    CMa    Was faint for 2 nights (October 8 and 9, 1962).
EY    CMa    P var, Delta(m) var [03960]. The main wave is superimposed
             by secondary ones (P = 0.2033d and 0.1690d); beat effect,
             Pb ~2.00d [07243].
EZ    CMa    SB. In the centre of the ring HII region S 308. Member of
             the open cluster collinder 121. Epoch of Max light is
             given. The companion is probably a neutron star. The shape
             of the light curve, Delta(m), phases of maxima and minima
             and mean light vary from one observational season to
             another.
FF    CMa    Min II 7.6. Elements should be improved. Member of the
             open cluster Cr 132a.
FM    CMa    Min II is almost as deep as Min I [06585].
FN    CMa    VB (6.3m,  7.5m, 0.561", 115.8deg, 1978.15). Range of
             combined light variation is given in the Table.
             Associated with the nebula vB 95. According to [06135],
             the period considerably differs  from the tabulated value.
FQ    CMa    Min II 9.7.
FR    CMa    ADS 4978 AB (6.2m, 10.4m, 4", 23deg; C 11.62m, 56").
FS    CMa    Extended shell of gas and dust. Emissions of [FeII],
             [NiII], [CrII], [SII], [OI], FeII. IR excess
             (1.6 - 20 mkm). P Cyg profiles of Balmer lines vary in the
             time scale of hours. Brightness varies from night to night
             by 0.1m and during a night by 0.03m, sometimes in
             correlation with spectral changes [06636]. Spectral
             studies [07250, 07251, 07253].
FT    CMa    VB A (B 12.58m, 36", 97deg).
FU    CMa    VB A (B 14.7m, 14", 230deg, 1897; C 11.07m, 40", 225deg).
FW    CMa    VR var, P = 31.9045d [06154].
FZ    CMa    Min II 8.44. In the HII region S 295, in the association
             CMa OB1.
GG    CMa    Member of the open cluster Cr 132a.
GU    CMa    ADS 5713 AB (7.5m, 8.2m, 0.6", 187deg, 1919). SB?
             In the HII region S 293.
GY    CMa    According to [08380], does not vary.
GZ    CMa    SB2.
HK    CMa    Epoch of Min is given.
HL    CMa    1E 0643.0-1648. SB (P ~0.217d); Lx/Lopt var (0.002 - 1).
IU    CMa    Type LBV: is also possible.
MO    CMa    The amplitude can have been overestimated (M. Grenon, private
             communication).
NO    CMa    Type LBV: is also possible.
bet   CMa    In 1971 - 72 the observations were described by the
             combination of the tabulated elements (period P1) and the
             following systems of elements:
             Max = 2441296.0705 + 0.251300d*E, (P2);
             Max = 2441296.032 + 0.23904d*E, (P3);
             Max = 2441296.065 + 0.12501d*E, (P1/2);
             Max = 2441296.124 + 0.12565d*E, (P2/2).
             Beat periods:  49.198d, 5.442d, 4.900d.
             Since 1908 P1 increases, P2 decreases. 12 overtone and
             resonance periods were found in [03454].
ksi 1 CMa    ADS 5176 A (B 14.5m, 25", 147deg; C 14.0m, 29", 303deg,
             1897).
sig   CMa    ADS 5719 A (14.2m, 11", 153deg, 1926).
tau   CMa    SB, Porb = 154.90d.
ome   CMa    SB?
R     CMi    SC4/10e.
T     CMi    P var. Max = 2422456 + 324.2d*E (JD2416610 -
             22800); Max = 2430896 + 311.2d*E (JD2423090 -
             30900); since JD2430900 - see Table.
U     CMi    There is a hump on the ascending branch looking sometimes
             as a secondary maximum. The light curve for 1904 - 1970
             [07368].
X     CMi    P var? Delta(S) = 3.
RS    CMi    d = 0.02P:.
RX    CMi    Min II 14.6; Min II - Min I = 0.52P:.
RY    CMi    Min II 12.0:.
SX    CMi    DI <= 0.12P. Min II 13.6.
SY    CMi    P var. Max = 2425234.682 + 0.565900d*E (JD2425234 - 708);
             since JD2436586 - see Table.
TU    CMi    Min II 15.1.
TW    CMi    Min II 15.6.
TX    CMi    Min II 14.7.
UZ    CMi    Min II 12.1.
XZ    CMi    Min II 9.88. P var?
YY    CMi    Min II 8.88.
YZ    CMi    mu = 0.604", P = 221.4deg. Epoch of Min is given. P var;
             additional term: -0.00003919514d*E*(E + 1)/2. Periodical
             light variations with the amplitude 0.12m (11.26 - 11.38 V)
             are superimposed by strong flares.
AG    CMi    P var. Min = 2434698.670 + 1.6645729d*E (JD2426350 -
             34740) [01727]. Since JD2437650 - see Table.
AH    CMi    EW?
AK    CMi    Min II 10.3; Min II - Min I = 0.55P. P var. Min I =
             2425352.348 + 0.56589534d*E (JD2424880 -
             35550) [01728]. Since JD2435600 - see Table.
AL    CMi    Observations in the interval JD2424880 - 25950 are
             represented by the elements: Max = 2425243.631 + 0.55050d*E.
             Since JD2436590  -  see Table.
AM    CMi    Min II 10.5.
AN    CMi    d = 0.02P:.
AO    CMi    d = 0.01P:. Min II 14.5.
BF    CMi    Depth of Min II 0.05m:.
BO    CMi    Several episodes of outburst-like activity.
RS    Cap    Mean brightness varies with P = 3360d.
RT    Cap    VB A (B 15m, 26", 227deg).
RU    Cap    VB A (B 13.6m, 1.6", 86deg).
RV    Cap    <P> var: Max = 2424334.6612 + 0.44775262d*E
             (JD2417400 - 33610) [00323]. Since JD2433850 - see Table.
             Light curve and period vary with the Blazhko effect
             period Pi = 225.5d [06464]. Semiamplitude  of deviations
             from linear elements is +-0.032d. 0.14P <= M - m <= 0.25P.
             (k - b)2 = 0.05.
RW    Cap    d = 0.020P. Min II 9.9. P var. Min I  = 2418924.594 +
             3.3923922d*E (JD2418920 - 24000) [06774];
             Min I  = 2424003.014 + 3.3923457d*E (JD2424000 -
             34500) [02389]; since JD2435400 - see Table.
RX    Cap    Min II 12.5.
RY    Cap    VB B (A 7.1m, F0; B 6.6", 90deg; C 12.0m, 8.5", 58deg).
TV    Cap    <P> = 67d [01331].
TW    Cap    P var. P = 28.6421871d (JD2414000 - 17600);
             P = 28.61700115d (JD2417600 - 24000) [01331];
             Max = 2426211.90 + 28.59497d*E (JD2421400 -
             26200) [02390]; Max = 2435664.8 + 28.5578d*E
             (JD2426210 - 37500) [02309]; since JD2437500 - see Table.
             0.14P <= M - m <= 0.40P. [Fe/H] =  -0.72.
TY    Cap    Min II 10.6. P var. Min I hel = 2432017.956 + 1.423466D*E
             (JD2425500 - 35000); since JD2435000 - see Table.
UW    Cap    Min II 11.5; Min II - Min I = 0.5P. P var? Min I =
             2434627.290 + 1.399118d*E (JD2427000 - 35000);
             since JD243500 - see Table.
YZ    Cap    (k - b)2 = 0.08.
AD    Cap    Outside eclipses B - V =  +1.00. P var?
AE    Cap    Mean brightness varies with P = 2300d.
BH    Cap    Type RR: is also possible.
BN    Cap    The variability may be due to the fainter (B) component.
del   Cap    VB A (B 15.8m, 69", 94deg; C 12.7m, 119", 302deg,
             1911); mu = 0.391", P = 138.8deg. Min II 2.90.
             The light curve shape var? [03305].
eps   Cap    VB A (B 9.52m, 68.7", 47deg).
R     Car    VB A (B 12m, 2.1", 138deg). H2O, SiO maser.
U     Car    P var. Max = 2429023.80 + 38.753d*E (JD2415000 -
             29500); since JD2429500 - see Table.
V     Car    The light curve shape var?
X     Car    Min II 8.6.
Y     Car    VB A (B 12.22m, 15"; C 12.96m, 30"). SB (P = 400 - 600d)
             [05119]. The fundamental mode period P0 is given in the
             Table (A = 0.58m). The first overtone period P1 = 2.55954d
             [05119] (A = 0.28m). P1/P0 = 0.7032.
RR    Car    P var. <P> = 154d (JD2421500 - 23500); <P> = 259d
             (JD2426400 - 30100); <P> = 154d (JD2430400 - 33100).
             S6.5/1- .
RT    Car    In the region of the cluster Tr 15.
RY    Car    There is a close companion 14.3 pg. P var.
             Max = 2418475 + 416d*E (JD2415140 - 18500);
             Max = 2429901 + 417.3d*E (JD2423600 - 32900);
             since JD2434100 - see Table.
ST    Car    Depth of Min II 0.27m.
SW    Car    Depth of Min II 0.05m.
SZ    Car    In the region of the cluster NGC 3114.
TX    Car    The light curve shape var?
TZ    Car    Mean brightness varies with P = 1183d; the amplitude of
             the short cycle is large in mean brightness maximum and
             small during its minimum.
UX    Car    In the region of the cluster IC 2581.
VV    Car    In the region of the very poor cluster N 99 [07374]
             (10h 36.0m -58deg 56', 1950.0) embedded in a nebula.
VY    Car    VB A (B 11.07m; B 9V:, 10", 150deg). P var.
             Nonlinear term: -0.000021d*E**2 (JD2410000 - 44200).
             The latest observations may be represented also by linear
             elements: Max = 2444161.16 + 18.9138d*E
             (JD2441000 - 44200). [A/H] = 0.4.
WZ    Car    P var. Max = 2419981.099 + 23.000945d*E (JD2410000 - 20000)
             [00025]; Max = 2423984.12 + 23.0054d*E (JD2419800 - 25500)
             [00322]; Max = 2434914.86 + 23.0075d*E + 0.000025d*E**2
             (JD2434500 - 41200) [02309]; since JD2434500 - see also
             Table.
XX    Car    P var. Max = 2420769.703 + 15.723704d*E (JD2410000 - 22500)
             [00025]; P = 15.7196d (JD2423000 - 30000) [00003]; since
             JD2434500 - see Table; elements given in the Table contain
             a nonlinear term: -0.0000034d*E**2.
XY    Car    [A/H] = 0.1.
XZ    Car    [A/H] = 0.2.
YZ    Car    P var. Nonlinear term: +0.0000022d*E**2. [A/H] = -0.1.
AE    Car    In the region of the cluster NGC 3532.
AF    Car    P var. Max = 2434532 + 433.7d*E (JD2420200 - 34600); since
             JD2435000 - see Table.
AG    Car    Central star of the low-excitation planetary nebula
             P.K.289-0.1 ejected probably during a nova-like outburst
             of the star about 1000 years ago [07052, 07113].
AS    Car    d = 0.025P.
AW    Car    d = 0.015P.
BL    Car    In the region of the cluster Tr 16.
BO    Car    VB A (B 11.05m V, B8III, 10", 41deg). In the region of
             the cluster Tr 15. Cluster non-member.
BP    Car    P = 4.82246d?
BS    Car    In the region of the cluster IC 2602. Min II 15.3.
BZ    Car    Mean brightness possibly varies with P = 1800d.
CD    Car    In the centre of the cluster Cr 236.
CF    Car    In the region of the cluster NGC 3496.
CI    Car    In the region of the cluster NGC 3572. d = 0.021P?
CO    Car    d = 0.024P?
CV    Car    d = 0.046P. Depth of Min II 0.05m.
DE    Car    d = 0.016P?
DH    Car    VB B (A 15.2m V; B 13", 350deg). B - V = +0.90m
             (Min brightness).
DI    Car    Besides Cepheid-like light variations with the amplitude
             1.7m and elements Max = 2438553.70 + 29.210d*E
             (JD2438465 - 40300) [05324] large weakenings of brightness
             are observed [04678]. At Max B - V = +1.34.
DK    Car    d = 0.07P.
DM    Car    d = 0.040P.
DP    Car    d = 0.034P. Min II 13.1.
DS    Car    d = 0.03P.
DU    Car    In the region of the cluster IC 2602.
DW    Car    In the region of the cluster Cr 228. Min II 10.3.
EF    Car    d = 0.04P.
EG    Car    In the region of the cluster NGC 3532.
EH    Car    VB A (B 15", 320deg).
EK    Car    In the region of the cluster NGC 3532.
EM    Car    Min II 8.9.
EN    Car    In the region of the cluster Tr 18.
EQ    Car    d = 0.030P. Min II 13.7.
ER    Car    In the region of the cluster NGC 3532.
ES    Car    In the region of the cluster NGC 3572.
EZ    Car    Min II 9.8.
FI    Car    P var. Max = 2425446.81 + 13.4542d*E (JD2423790 - 35300)
             [00046, 02309]. Since JD2435300 - see Table.
FK    Car    VB.
FO    Car    VB A (B 14m, 7", 90deg). P var. Max = 2434922.531 +
             10.3559d*E (JD2423700 - 35300) [06006]; since JD2436000
             - see Table. B - V: +1.13, +1.43.
FP    Car    d = 0.01P:.
FQ    Car    In the region of the cluster Tr 18.
FS    Car    In the region of the very poor cluster N 99 [07374] (10h
             36.0m -58deg 56', 1950.0) embedded in a nebula. Min II
             10.9.
FT    Car    According to [02197] spectrum C. Misidentification is
             possible.
FV    Car    VB A (B 13m, 10", 135deg). P var. There are two additional
             terms in the elements given in the Table:
             -0.1065d*10**(-7)*E**2 - 0.584d*10**(-11)*E**3.
             d = 0.02P:. Min II 13.0.
GG    Car    Min II 9.5. Gas and dust envelope.
GH    Car    In the region of the cluster Tr 18.
GK    Car    In the region of the cluster Tr 19. Min II 13.2.
GL    Car    In the region of the cluster NGC 3572. Min II 10.31.
             System with the apsidal motion; e = 0.157, omega = 99deg.
             There are sinusoidal terms in the elements for Min I given
             in the Table: +0.121d sin(0.094389deg*E) -
             0.007d sin(0.188778deg*E);
             Min II = 2424263.236 + 2.4222338d*E -
             0.121d sin(0.094389deg*E) - 0.007d sin(0.188778deg*E).
             DII = 0.17P.
GM    Car    In the region of the very poor cluster N 99 [07374] (10h
             36.0m -58deg 56', 1950.0) embedded in a nebula.
             Min II 9.22.
GN    Car    Min II 12.1.
GO    Car    VB A (B 15", 60deg).
GP    Car    Min II 12.8.
GQ    Car    Min II 13.5.
GR    Car    Min II 14.0; Min II - Min I = 0.316P; DII = 0.05P.
GV    Car    Possible member of the cluster NGC 3532. Min II 9.1.
GW    Car    Min II 9.9.
GZ    Car    Light elements for the fundamental mode oscillation with
             an amplitude 0.16m are given in the Table. For the first
             overtone oscillation with an amplitude 0.07m
             Max = 2440742.4 + 2.93424d*E. Epochs of maxima and
             amplitudes are given according to [05175].
HH    Car    VB A (B 13.0m, 5", 260deg; C 11.11m, 13", 337deg; D 12.65m,
             15", 7deg). d = 0.02P. Min II 10.66. P var [08094].
             Min I hel = 2430860.162 + 3.2315393d*E (JD2427590 - 35260)
             [05292]. Possible current elements are given in the Table.
HI    Car    Min II 10.8.
HK    Car    VB A (B 12.5m, 4"). Range of combined brightness variation
             is given.
HL    Car    d = 0.03P:.
HN    Car    Min II 12.5.
HP    Car    VB A (B 9.1m, 0.4", 178deg). Min II 9.3. Elements should
             be corrected [08083].
HQ    Car    B - V: +0.63,  +1.04.
HR    Car    Spectrum description  [01914, 06466].
HT    Car    In the region of the cluster IC 2581. Min II 14.0.
HV    Car    d = 0.026P. Min II 14.2.
HW    Car    Epoch of Min is given.
HX    Car    Min II 14.5.
IK    Car    In the region of the cluster NGC 2602.
IL    Car    Min II 14.4.
IN    Car    It is possible that the period must be doubled.
IQ    Car    In the region of the cluster NGC 3532.
IR    Car    In the region of the cluster NGC 3532. Min II 12.6.
IS    Car    Min II 14.0.
IU    Car    (k - b)2 = 0.02.
IW    Car    Mean brightness varies with the period close to 1500d, the
             amplitude of main oscillations - from 1.3m to 0.3m.
IX    Car    In the centre of a bright nebula with the diameter 2.4'.
IZ    Car    Declination in [00085] is wrong by 3deg. Identical to
             V336 Car, see [06316].
KQ    Car    Min II 10.3.
KU    Car    Min II 11.6.
MP    Car    VB A (B 16m, 180deg).
MZ    Car    sf component of a close pair.
OO    Car    Min II 14.7.
OV    Car    Min II 13.5.
OY    Car    Eclipse elements:
             Min I hel = 2443993.553241 + 0.0631209247d*E [05185];
             D = 0.050P, d = 0.044P. The hump on the light curve is
             observed at the phase of 0.75P. Depth of Min I varies
             between 1.48m and 2.47m.
PT    Car    Min II 13.0:.
PX    Car    Min II 10.10.
QR    Car    Min II 10.4.
QS    Car    Min II 9.3.
QU    Car    HDE 310376 (HA 112, 173). Flickering resembles V818 Sco.
             Variations by 0.2m in 90s were observed. No periodicity
             was found. Emission lines He II 4686, CIV - NIII 4630 -
             4650 and sometimes weak hydrogen absoptions (corresponding
             to A or B type) are noticeable in the spectrum [05643].
QX    Car    Min II 7.02.
QY    Car    In the open cluster No.90 [07374].
QZ    Car    In the eta Carina nebula, possible member of the cluster
             Collinder 228. Min II 6.43. Two SB1 systems (A and B),
             B is eclipsing (A: SB1, P = 20.73d, O9.5 I,
             Delta(m) = 0.6m). Combined brightness is given.
V0341 Car    In the variable reflecting nebula IC 2220. In the region
             of the open cluster NGC 2516. IR excess.
V0343 Car    VB. SB (P = 133.92d).
V0347 Car    Deep Min II.
V0348 Car    In the open cluster IC 2581. Min II 8.9.
V0354 Car    Very red.
V0356 Car    Member of the cluster NGC 2516.
V0357 Car    SB (P = 6.74483d [04627]).
V0361 Car    In the region of the cluster NGC 3293.
V0365 Car    In the region of the cluster NGC 3532.
V0367 Car    Min II 7.54.
V0373 Car    Member of the cluster NGC 2516.
V0374 Car    Member of the cluster NGC 2516.
V0375 Car    P = 0.264d or 0.359d.
V0376 Car    VB A (B 6.83m, B 9.5V, 41", 75deg).
V0378 Car    In the open cluster NGC 3293.
V0379 Car    In the open cluster NGC 3293.
V0380 Car    In the open cluster NGC 3293.
V0381 Car    In the open cluster NGC 3293.
V0382 Car    In the region of the cluster NGC 3532.
V0385 Car    Depth of Min II 0.04m. Surrounded by a ring nebula RCW 58.
V0491 Car    Mean magnitude 9.69.
V0493 Car    SB, Porb = 3.368d.
V0498 Car    Type BE: is also possible.
V0534 Car    Flare-like activity.
eta   Car    In the emission nebula NGC 3372 in the region of the
             cluster Tr 16. A very massive young star surrounded by an
             expanding gas and dust shell with the diameter 2" at 2mu
             and 6.5" at 12.2mu. Maximum brightness was observed in
             1843. Since 1880 varies in the range 5.9 - 7.9 V. In the
             interval JD2434000 - 41000 Max = 2434037 + 1110d*E. There
             are emission lines of H, HeI, FeII, [FeII], etc. in the
             spectrum. Description of the spectrum [05251, 07279].
             Soft X-ray source of variable intensity.
khi   Car    Soft X-ray source.
R     Cas    VB A (B 14.5m, 14", 273deg). SiO, OH maser;
             sometimes H2O emission.
T     Cas    SiO maser. ZrO bands in the infrared spectral region.
U     Cas    S4.5/4e.
W     Cas    SC5/9e.
X     Cas    P var: Max = 2426650 + 432.32d*E (JD2416750 - 27060);
             Max = 2432870 + 413.6d*E (JD2427060 - 32870);
             Max = 2437948 + 423.0d*E (JD2432870 - 39210).
             Current elements are given in the Table.
Y     Cas    OH, H2O emission; SiO maser.
Z     Cas    SiO maser.
RS    Cas    P var. Max = 2416942.16 + 6.29552d*E (JD2412650 - 34900)
             [03317]. Since JD2434900 - see Table.
RV    Cas    There are signs of Se type in the spectrum [03383].
RW    Cas    P var. Max = 2421354.22 + 14.8004d*E (JD2417000 - 30000).
             Since JD2430000 - see Table. [A/H] = 0.3.
RX    Cas    Unigue rapidly evolving eclipsing system. 9.12<=Min II<=9.49;
             Min II - Min I = 0.5070P. P var. Nonlinear term:
             +1.017d*10**(-5)*E**2. Observations may be represented
             also by three systems of elements: Min I =
             2416250.889 + 32.31481d*E (0 <= E <= 286,
             JD2416250 - 25482); Min I = 2416248.835 + 32.32145d*E
             (331 <= E <= 554, JD2426940 - 34155);
             Min I = 2416244.990 + 32.32765d*E (734 <= E <= 876,
             JD2439970 - 44570). Brightness of the system out of
             eclipses periodically varies within 8.6m - 9.0m with
             elements Max = 2416198 + 516.06d*E [05036]. Max - Min =
             233d = 0.45P [00881]. Strong emissions of H, NV, CIV,
             SIIV, FeIII. Powerful gaseous stream and accretion
             phenomena are possible.
RY    Cas    [A/H] = 0.0.
RZ    Cas    Min II 6.26. The light curve shape var; d var
             (0.000P <=  d <= 0.009P). P var, variations are irregular.
             Mean elements based on visual and photographic
             observations: Min I = 2416886.8806 + 1.195253065d*E
             (JD2416800 - 26700) [08820], Min I = 2432820.7853 +
             1.1952517d*E (JD2426700 - 34000) [00938]. From
             photoelectric observations: Min I = 2432115.5827 +
             1.1952472d*E (JD2429870 - 30400); Min I =
             2432085.7011 + 1.195259d*E (JD2432000 - 32460);
             Min I = 2434349.5130 + 1.1952525d*E (JD2432450 - 34420);
             Min I = 2434703.3035 + 1.195238d*E (JD2434420 - 34705);
             Min I = 2435934.4087 + 1.1952499d*E (JD2434705 - 35950);
             Min I = 2438829.2818 + 1.195243d*E (JD2436800 - 39100);
             Min I = 2440182.3089 + 1.195259d*E (JD2439380 - 40200);
             Min I = 2441333.3257 + 1.195244d*E (JD2440500 - 41350);
             Min I = 2442327.7798 + 1.1952521d*E (JD2441550 - 42350);
             since JD2442850 - see Table.
SU    Cas    [A/H] = -0.1.
SV    Cas    P var. Max = 2421839 + 279.3d*E (JD2417600 -
             21900); Max = 2430450 + 281.7d*E (JD2422500 -
             31900); since JD2432600 - see Table.
SX    Cas    VB A (B 11.5m, 19", 250deg, 1966). Min II 9.32. The light
             curve shape var. DII = 0.171P:, dI = 0.036P, dII = 0.050P.
             P var. Min I = 2433963.267 + 36.56727d*E (JD2418000 -
             37000); since JD2438700 - see Table. Strong emissions
             of H, NV, CIV, SIIV, FeIII. Gaseous streams and accretion
             phenomena.
SY    Cas    VB? P var. Max = 2417911.547 + 4.070969d*E
             (JD2417000 - 34000); since JD2434000 - see Table.
SZ    Cas    P var. Max = 2421261.66 + 13.6009d*E (JD2416700 - 21260);
             Max = 2426650.20 + 13.6072d*E (JD2421260 - 27170) [08821];
             Max = 2429727.240 + 13.61744d*E (JD2427170 - 33050);
             Max = 2436810.92 + 13.62655d*E (JD2433050 - 38720);
             since JD2438720 - see Table. [A/H] = -0.6.
TU    Cas    Fundamental mode period P0 is given in the Table; the
             corresponding amplitude is 0.69m. First-overtone period
             P1 = 1.51830d; the corresponding mean amplitude decreased
             from 0.4m to 0.25m during 67 years [05078]. P1/P0 = 0.71.
             M - m var (0.17P <=  M - m <= 0.35P).
TV    Cas    d = 0.01P. Min II 7.34. The light curve shape var.
             Period of these variations - 600d [08822]. P var. Mean
             elements based on visual and photographic observations:
             Min I = 2432827.7665 + 1.81260983d*E (JD2415650 - 32800)
             [01926]. From photoelectric observations Min I =
             2432827.7665 + 1.8126142d*E (JD2432800 - 36490);
             Min I = 2436483.8091 + 1.81255d*E (JD2436480 - 36980);
             Min I = 2438472.2386 + 1.81263d*E (JD2437000 - 38500);
             Min I = 2438829.3230 + 1.8126048d*E (JD2438470 - 41750);
             since JD2441750 - see Table.
TW    Cas    Min II 8.40.
TX    Cas    Min II 9.6.
TY    Cas    P var. Max = 2419260 + 545.0d*E (JD2419200 - 25300);
             Max = 2428965 + 623.8d*E (JD2427000 - 41500);
             since JD2441500 - see Table.
UU    Cas    Min II 10.5.
UZ    Cas    [A/H] = -0.3.
VV    Cas    P var. Max = 2422514.16 + 6.207510d*E (JD2417000 - 32500);
             since JD2432500 - see Table. [A/H] = -0.2.
VW    Cas    [A/H] = 0.0.
WY    Cas    In the region of the cluster NGC 7789.
             The spectrum of the G type star is seen in minimum light
             [03502]. The existence of a physical companion is possible.
             S6/6-e.
WZ    Cas    VB A (optical companion B 8.7m, 58", 89deg). SC7/10e.
             Light variations are sometimes taking place with doubled
             period.
XX    Cas    Min II 10.2.
YZ    Cas    VB A (B 11.23m, 35", 160deg). d = 0.045P. Min II 5.78.
ZZ    Cas    Min II 10.9.
AB    Cas    EA/SD. Min II 10.28. P var. Min I = 2430755.678 +
             1.366863d*E (JD2425400 - 33150); Min I =
             2433616.532 + 1.366876d*E (JD2433150 - 37000);
             Min I = 2440475.5216 + 1.3668783d*E (JD2437000 -
             41600); since JD2441600 - see Table.
             The A3 component is a DSCT type variable with the elements:
             Max hel = 2444912.1759 + 0.0582874d*E [08825]; amplitude
             of pulsations Delta(V) var (0.03m <= Delta(V) <= 0.09m).
AE    Cas    Min II 12.8.
AH    Cas    Min II 13.3.
AL    Cas    Min II 13.6.
AO    Cas    Min II 6.24. The light curve shape var. P var?
AQ    Cas    Min II 10.4.
AR    Cas    VB A (B 9.3m, 1.0", 336deg; C 8.2m, 75", 269deg;
             D 9.8m, 76", 268deg; E 11.28m, 43", 115deg; F 11.06m, 69",
             338deg; G 11.11m, 67", 348deg). Min II 4.86;
             Min II - Min I = 0.614P; DII = 0.076P; dII = 0.037P.
AS    Cas    VB A (B 15.5m, 3", 45deg).
             Fundamental mode period P0 is given in the Table; the
             corresponding amplitude is 0.59m. First-overtone period
             P1 = 2.2909d; amplitude of oscillations with this period
             is 0.13m. P1/P0 = 0.76.
AX    Cas    Min II 12.9.
AZ    Cas    B - V: +1.78, +2.20. D = 110d, d = 88d = 0.026P.
BD    Cas    B - V: +1.50, +1.61. P var. Max = 2429124.84 +
             3.65129d*E (JD2415000 - 29130) [00915];
             since JD2429130 - see Table.
BE    Cas    VB A (B G, 25", 260deg).
BH    Cas    According to [00453] there are no variable stars on the
             place of BH Cas and in its surroundings.
BM    Cas    Min II 8.98. Shape of the light curve varies. P var.
             There is a periodic term in the elements:
             +2.6d*sin(7.11deg*E + 104deg).According to [00939], on the
             light curve cepheid-like variations are observed with
             P = 27d.
BN    Cas    Min II 13.4.
BS    Cas    Min II 12.6.
BU    Cas    D = 0.02P.
BY    Cas    In the region of the cluster NGC 663. P var.
             Max = 2416871.91 + 3.2218d*E (JD2416800 - 24860) [00921];
             Max = 2431929.60 + 3.221297d*E (JD2426900 - 34300);
             Max = 2438399.629 + 3.222588d*E (JD2436200 - 39400);
             since JD2439400 - see Table.
BZ    Cas    Min II 11.5.
CC    Cas    Min II 7.26. The light curve shape var? P var?
CE    CasA   Possible member of the cluster NGC 7790. VB A (B = CEb Cas,
             2.4", 265deg).
CE    CasB   VB B (A = CEa Cas). Possible member of the cluster NGC 7790.
CF    Cas    Possible member of the cluster NGC 7790. [A/H] = 0.1.
CG    Cas    In the region of the cluster NGC 7790.
CH    Cas    [A/H] = -0.5.
CQ    Cas    The slow oscillations are superimposed by more rapid ones
             with cycles from 110d to 250d.
CR    Cas    Min II 13.3.
CS    Cas    [A/H] = -0.4.
CV    Cas    Epochs given in [00922] are not represented by the elements
             given in the Table. P var?
CW    Cas    Min II 11.47. Shape of the light curve and depths of
             minima vary. P var. Min I = 2435745.6163 + 0.31886497d*E
             (JD2432400 - 41000) [03332]; since JD2441000 - see Table.
CY    Cas    [A/H] = -0.7.
DD    Cas    P var. Max = 2415612.45 + 9.807272d*E (JD2415600 - 18600);
             since JD2418600 - see Table. The star may be a member of a
             binary system with Porb = 8500d +- 1000d.
DF    Cas    In the region of the cluster NGC 1027.
DI    Cas    P var. Max = 2432068 + 371.7d*E (JD2417200 - 32100);
             since JD2432100 - see Table.
DL    Cas    Member of the cluster NGC 129. [A/H] = 0.0.
DN    Cas    Min II 10.13.
DO    Cas    Min II 8.61; dI = 0.08P.
DP    Cas    Min II 13.6.
DZ    Cas    Min II 12.0.
EG    Cas    Min II 13.1.
EK    Cas    Depth of Min II 0.05m.
EM    Cas    P var. Max = 2433132 + 283d*E (JD2427700 - 33150); since
             JD2433150 - see Table. Amplitude strongly varies.
EN    Cas    Min II 12.4. P var.
EP    Cas    Min II 11.4.
EQ    Cas    Min II 12.7. P var. Min I = 2432150.04 + 58.26d*E
             (JD2432200 - 34060) [03336]; since JD2436100 - see Table.
EY    Cas    Min II 14.5.
GG    Cas    d = 0.013P. Min II 9.99. P var? Min I = 2430188.468 +
             3.758738d*E (JD2424800 - 39500) [00936];
             since JD2439500 - see Table.
GK    Cas    Depth of Min II 0.05m.
GT    Cas    d = 0.02P.
GU    Cas    Min II 11.3. P var. Min I = 2428749.423 + 3.093329d*E
             (JD2417470 - 35480) [00941];
             Min I = 2437367.375 + 3.09325d*E (JD2435480 - 38750) [00001];
             since JD2438750 - see Table.
GZ    Cas    Mean magnitude varies with P = 800d.
             Max = 2428000 + 800d*E [00911].
HH    Cas    Epoch of Min is given. RV type is possible [00911].
HN    Cas    d = 0.038P.
HS    Cas    VB A (B 12m, 27", 15deg).
HT    Cas    Min hel = 2443727.93722 + 0.073647217d*E;
             D = 0.13P. Depth of eclipses between outbursts is ~2.4 V.
             Small quasi-periodic light oscillations with P = 100s.
             Spectrum description [06163].
HU    Cas    P var. Max = 2417525.075 + 0.41159875d*E (JD2411600 -
             28000); since JD2428000 - see Table.
IL    Cas    Depth of Min II 0.05m.
IR    Cas    Min II 11.5. P var. Min I = 2428750.2914 +
             0.68069178d*E (JD2417500 - 38400) [00098];
             since JD2438400 - see Table.
IS    Cas    Min II 12.2. P var. Min I = 2428776.262 +
             1.8415172d*E (JD2417400 - 29500) [00098];
             since JD2428000 - see Table.
IT    Cas    Min II 11.8; Min II - Min I = 0.553P; DII = 0.042P.
             Apsidal motion is possible.
IV    Cas    Min II 11.3. P var. Min I = 2428991.302 +
             0.9985232d*E (JD2416700 - 29000) [00098];
             Min I = 2431438.648 + 0.9985056d*E (JD2429000 -
             37700) [02263]; since JD2440000 - see Table.
IW    Cas    S4 +/6e.
IX    Cas    P var. Max = 2428749.39 + 9.15035d*E (JD2414700 -
             29500) [00098]; Max = 2428749.90 + 9.1363d*E
             (JD2428700 - 34350) [00944]; Max = 2437195.642 +
             9.14783d*E (JD2434350 - 39100) [05462];
             since JD2442000 - see Table. [A/H] = -0.4.
KL    Cas    Min II 12.3.
KO    Cas    P var. Max = 2425590 + 305.6d*E (JD2416700 - 26000);
             since JD2426000 - see Table.
KR    Cas    Min II 9.9.
LR    Cas    Min II 10.9.
LU    Cas    Min II 14.3?
LW    Cas    In the apex of a small (8") bright cometary nebula in the
             region of IC 1848. Novalike outburst was observed in the
             interval JD2433900 - 34800. Infrared and radioemission.
LX    Cas    In the region of the cluster Collinder 33. Min II 15.3;
             Min II - Min I = 0.47P; dI = 0.10P.
LY    Cas    In the region of the cluster Collinder 33. Min II 15.2.
MM    Cas    d = 0.08P: Min II 12.4.
MN    Cas    Min II 10.57.
MO    Cas    In the nebula NGC 7635. 10.2 - 13.1 I.
MP    Cas    In the nebula NGC 7635. 10.4 - 13.5 I.
MR    Cas    Min II 15.5.
MS    Cas    Min II 13.2.
MT    Cas    d = 0.04P. Min II 14.02.
MU    Cas    Min II 10.8.
MV    Cas    Min II 14.0.
MY    Cas    Min II 15.2. P var. Elements given in the Table are valid
             since JD2438500.
NN    Cas    Min II 14.0.
NT    Cas    Min II 14.4.
NU    Cas    Min II 13.4.
NV    Cas    d = 0.03P.
OP    Cas    P var. Max = 2429109.726 + 5.510019d*E (JD2427950 - 34670)
             [00176]; since JD2437000 - see Table.
OR    Cas    Min II 11.8. P var. Min I = 2429249.424 + 1.2457026d*E
             (JD2413800 - 34800) [00176]; since JD2432000 - see Table.
OX    Cas    In the region of the cluster NGC 381. d = 0.016P. Min II
             10.30; Min II - Min I = 0.512P. Apsidal motion [04524].
PR    Cas    P = 171d?
PV    Cas    Min II 10.36; Min II - Min I = 0.480P.
             Depth of Minima probably varies. P var. Min I =
             2428796.8142 + 1.75047346d*E (JD2415700 - 40000) [05302];
             since JD2440000 - see Table. Apsidal motion [06253]:
             Min II = 2428797.6894 + 1.75047346d*E -
             0.040d*sin(0.0075deg*(E - 3000)).
PX    Cas    Min II 15.0.
PY    Cas    Epoch of Min brighness is given. Similar to RV Tau by
             light curve shape [03348].
PZ    Cas    VB A (B 12.8m, WN 8:, 15", 100deg). OH, H2O emission.
QQ    Cas    Min II 10.8. P var. Min I = 2434330.169 + 2.142030d*E
             (JD2415700 - 30000) [02530]; since JD2430000 - see Table.
QX    Cas    In the region of the cluster NGC 7790. VB A (B 13.1m, 3").
             Min II 10.50; Min II - Min I = 0.37P; DII = 0.047P;
             dII = 0.018P.
V0336 Cas    Min II 13.6.
V0341 Cas    d = 0.031P.
V0344 Cas    Min II 13.4.
V0345 Cas    Min II 13.6.
V0346 Cas    The coordinates refer to the sp component of a wide pair,
             whereas the chart [02345] leads to the nf component. It is
             the sp component that is red and probably var.
V0357 Cas    Min II 13.6.
V0359 Cas    Min II 12.0.
V0360 Cas    Min II 12.3.
V0361 Cas    d = 0.051P.
V0363 Cas    Delta(S) = 1.
V0364 Cas    Min II 11.9.
V0365 Cas    S6/3- .
V0366 Cas    Min II 12.7. P var. Min I = 2435075.461 + 0.7292714d*E
             (JD2414600 - 35400) [02305]; since JD2434650 - see Table.
V0373 Cas    An unique close binary. Porb = 13.4192d [04627]. Epoch
             of Min I is given close to the epoch of one of
             conjunctions. Min II - Min I = 0.58P. Maxima are very
             sharp. Max - Min II = 0.25P. It is not excluded that the
             star is an eclipsing one with physical variability of
             components, but eclipses, if they exist, cause only a very
             small part of the observed light variations. Range of
             light variations is given according to [02651]. As a rule
             the amplitude is close to 0.1m.
V0374 Cas    Min II 12.1.
V0375 Cas    Min II 10.6.
V0377 Cas    VB (A 8.5m; B 9.4m, 2.1", 185deg, 1962).It is not known
             which component varies. According to [04005] the range
             of combined brightness variations is 0.26m.
             According to [07051], const.
V0380 Cas    d = 0.08P.
V0381 Cas    Min II 10.8.
V0388 Cas    Wolf 47 (mu = 0.82", p = 80deg). Faint component of a wide
             physical pair (p = 294") the bright component of
             which is the dM2 star Wolf 46 = BD+61deg 195 (9.4).
V0392 Cas    Min II 14.0. P var. Min I = 2429640.390 +
             4.54094d*E (JD2425300 - 29640); Min I =
             2429640.390 + 4.54064d*E (JD2429640 - 36900) [04027];
             since JD2436900 - see Table. Depth of Min var?
V0394 Cas    Min II 15.6.
V0396 Cas    Min II 10.2.
V0399 Cas    Min II 14.1.
V0401 Cas    Min II 15.7.
V0402 Cas    Min II 15.3.
V0406 Cas    Min II 16.8.
V0410 Cas    Bright in 1938 -39. Slow. Not red.
V0423 Cas    Min II 14.3.
V0427 Cas    Min II 13.7.
V0428 Cas    Red.
V0430 Cas    Northern component of a close pair. Red.
V0434 Cas    Red.
V0441 Cas    P = 351.2d?
V0442 Cas    d = 0.025P. P var? Since 1972 P = 3.592120d.
V0444 Cas    Min II 16.0. P var. Min I = 2438651.314 + 2.224808d*E
             (JD2432850 - 37300); since JD2437300 - see Table. Period
             variation may be cyclic. Mean elements:
             Min I = 2443194.258 + 2.224773d*E.
V0445 Cas    Min II 11.08.
V0448 Cas    Min II 15.0.
V0450 Cas    VB A (B 17.5m:, 3.4", 188deg). Range
             of combined light variations is given.
V0459 Cas    Min II 11.6.
V0466 Cas    In the region of the cluster NGC 457.
V0480 Cas    Min II 14.7.
V0482 Cas    VB A (B 10.0m, F 4 V, 6", 195deg; optical). P = 0.28292d?
V0497 Cas    In the region of the cluster IC 1848.
V0498 Cas    In the region of the cluster IC 1848.
V0499 Cas    In the region of the cluster IC 1848.
V0509 Cas    Pulsation of photosphere with P = 3 years.
             Tenuous shell ejected in 1975 is now falling back to
             the star.
V0518 Cas    In the region of the cluster Stock 2. Star N136 (Stock 208).
V0520 Cas    Min II 13.1. P var. Min I = 2439069.559 + 0.489832d*E
             (JD2438580 - 40850); since JD2441150 - see Table.
V0521 Cas    Member of the cluster NGC 7789.
V0523 Cas    Min II 11.34. P var. Min I = 2432054.555 +
             0.2336882d*E (JD2428545 - 33570) [07008];
             Min I = 2439029.461 + 0.23368912d*E (JD2439000 - 41300)
             [07387]; since JD2440480 - see Table.
V0524 Cas    OH, H2O emission. P = 163d?, 191d? 259d?, 620d?
V0526 Cas    Two oscillations are superimposed: P1 = 0.0526d (A1 =
             0.0036m), P2 = 0.0396d (A2 = 0.0056m); P2/P1 = 0.753.
V0527 Cas    Min II 13.5; Min II - Min I = 0.52P.
V0532 Cas    In the region of the cluster NGC 7789.
V0533 Cas    In the region of the cluster NGC 7789.
V0536 Cas    P var. Max = 2438700.262 + 0.395674d*E
             (JD2438580 - 39150); Max = 2441186.333 +
             0.395683D*E (JD2440070 - 41250);
             since JD2441500 - see Table.
V0540 Cas    Epoch of Max (U) is given.
V0541 Cas    Min II 11.0.
V0542 Cas    In the region of the cluster NGC 7789.
V0544 Cas    Elements given in the Table are valid since JD2428000.
V0546 Cas    In the region of the cluster NGC 103. Min II 14.8.
V0547 Cas    VB A (B 12.4m, M4.5, 2.8", 93deg). Astrometric binary
             (A = 0.12", P = 15.9a); mu = 1.75", P = 98deg.
             Variation of combined light is given.
V0551 Cas    P = 45.5d?/57d?/67.5d?.
V0554 Cas    P >= 3500d? D = 400d?
V0559 Cas    VB A (B 7.7m, 0.25", 34deg, 1976). Min II 7.21.
V0566 Cas    VB A (B 8.3m, 1.4", 194deg, 1965).
V0569 Cas    10.0 - 14.7 I.
V0589 Cas    In the cluster NGC 663.
V0592 Cas    White dwarf. Rapid non-periodic fluctuations of brightness
             on a time scale of several minutes.
V0598 Cas    VB A (B 12m, 19", 0deg). P = 2.825d? [02560].
V0615 Cas    Variable radio source on 10.5 GHz; gamma - and X-ray
             source?
V0627 Cas    H2O emission.
V0635 Cas    4U 0115 + 634. SB (P = 24.3162d).
             Pulsar period P = 3.6136s.
V0638 Cas    Epoch of Min is given.
V0742 Cas    SB, Porb = 55.9212d.
V0745 Cas    Component B of the double system observed brighter than in the
             Hipparcos Input Catalogue.
V0746 Cas    SB, Porb = 27.8d.
V0747 Cas    VB. The variability may be due to the fainter component.
alf   Cas    VB A (B 14.5m, 17.6", 272deg; C 13.5m, 38", 105deg;
             D 8.5m, 64.4", 280deg.)
bet   Cas    VB A (B 13.7m, 31.3", 243deg); SB (P = 27d).
             [Fe/H] = 0.64.
gam   Cas    VB A (B 11.0m, 2.2", 248deg; C 13.0m, 52.2", 348deg).
             In HII region S 185. X-ray source MX 0053 + 60.
             v sin i = 310 km/s.
del   Cas    VB A (B 11.5m, 31.7", 66deg). Min II 2.75. Min II - Min I =
             361d. The elements given in the Table are still not
             confirmed by anyone.
iot   Cas    VB A (B 6.89m, 2.3", 239deg; C 8.40m, 7.2", 114deg).
             Astrometric binary (a = 0.113", P = 52.4a). Max (V) - Max
             (lambda 1550) = 0.4P; A (lambda 1550) = 0.40m. The range
             of total brightness variation of components A and
             B is given.
kap   Cas    P = 0.09028d, P(Vr) = 0.14035d [02588]; P = 7d [08876].
omi   Cas    VB A (B 11.7m, 33.6", 303deg). SB1 (P = 1033d);
             V sin I = 220 km/s.
pi    Cas    SB, Porb = 1.9642d.
rho   Cas    Usually varies within the limits 4.4m - 5.2m V.
             In November 1945 the peculiar decrease of brightness began
             lasting for 165d and in September 1946 the star reached
             the middle of the deepest minimum (JD2432070) lasting for
             320d. Then the brightness began to increase symmetrically
             and by July 1947 the star attained its normal brightness
             [00957]. Photographic magnitudes varied in the limits
             5.4m - 8.3m. Spectrum description [08878].
B     Cas    Tycho Brahe's supernova. Stellar object is not identified
             optically up to now.
R     Cen    VB A (B 12m, 28", 218deg). Epoch
             of Min I is given. Min I 0.00P, Max I 0.23P, Min II
             0.47P, Max II 0.64P. <Max I> 5.8, <Max II> 6.0,
             <Min I> 11.1, <Min II> 8.3. P var. P = 561.3d
             before 1918; since 1918 - see Table. H2O maser.
V     Cen    In the field of the open cluster NGC 5662.
Z     Cen    SN 1895 (NGC 5253).
RR    Cen    Min II 7.63. dII = 0.08P. P var. Min I = 2424231.0910 +
             0.60568807d*E + 2.31d*10**(-10)*E**2 (JD2414170 -
             33470) [00006]. Current elements - see Table.
RS    Cen    A 1118-61?
RT    Cen    P var.
RZ    Cen    Min II 9.4.
SS    Cen    Min II 9.5.
ST    Cen    Min II 11.30, DII = 0.22P. Max II (before
             Min I) 10.65.
SU    Cen    Min II 9.2.
SV    Cen    Min II 9.45. Delta(m) var. P var. Min = 2433053.358 +
             1.6594795d*E - 7.61d*10**(-8)*E**2 (JD2412608 - 42097).
             Cyclic (32a - 33.6a) period variations were noted in
             [00009, 05212]. Since 1978 - see Table. P Cyg profiles in
             the spectrum.
SX    Cen    For mean light Max = 2426835 + 615d*E.
SY    Cen    d = 0.05P.
SZ    Cen    VB. Min II 8.7.
TX    Cen    VB? B - V: +1.39, +2.11.
TZ    Cen    The co-ordinates in the Table are based on [00015].
             According to [00016], no star brighter than 14m was found
             in this position. The co-ordinates in [00015] may be in
             error.
UW    Cen    IR excess.In Max varies semiregularly, P ~42d [08832].
UZ    Cen    VB A (B 13.8m, 4", 191deg). Max II = 2440746.2 +
             2.35529d*E.
VW    Cen    VB A (B ~15m?, ~8", ~180deg). B - V: +1.01, +1.71.
             [A/H] = 0.3.
VZ    Cen    Min II 8.4.
WX    Cen    <B - V> ~ +0.45, <U - B> ~ -0.72.
             Proposed as an optical counterpart of the transient X-ray
             source Cen X-2 [05314], though no optical bursts were
             observed.
WZ    Cen    Min II 14.2.
ZZ    Cen    VB C (A 9.4m, B9; B 10.8m, 8", 314deg; C = ZZ Cen,
             9", 259deg; D = AA Cen, 9", 110deg).
AA    Cen    VB D (see ZZ Cen).
AB    Cen    d = 0.05P.
AP    Cen    Epoch of Min is given.
AS    Cen    Min II 13.2.
AV    Cen    Min II 14.1.
AZ    Cen    The shape of the light curve varies.
BD    Cen    Min II 10.7.
BF    Cen    In the field of the open cluster NGC 3766. Min II 8.8.
BG    Cen    Min II 12.3.
BH    Cen    In the open cluster IC 2994. Min II 8.8.
BI    Cen    Delta(S) = 2.
BK    Cen    P2 = 2.236d, A1 = 0.54m, A2 = 0.22m [08835].
BV    Cen    The mean cycle between outbursts <= 149.4d [07301]. The
             tabulated elements correspond to Max of the eclipsing
             light curve, phi (Min) = 0.25P. The range of the eclipsing
             variability is 12.8 - 13.3.
CN    Cen    Min II 13.3.
DI    Cen    Min II 12.3, Min II - Min I = 0.494P, DII = 0.08P:.
DT    Cen    Red.
DX    Cen    The P star in a pair.
DY    Cen    All spectral lines are very weak. No IR excess. The
             photometric behaviour outside major Min is described in
             [08836].
EP    Cen    Min II 11.5.
EU    Cen    The P star in a pair.
GI    Cen    In the field of the globular cluster NGC 5286.
GM    Cen    The chart in [06286] is wrong.
IQ    Cen    d = 0.04P.
IW    Cen    Min II 12.1.
IX    Cen    In the field of the open cluster NGC 3706.
IY    Cen    In the field of the open cluster IC 2944.
IZ    Cen    <B - V> = 1.7.
KK    Cen    B - V: +1.08, +1.62.
KM    Cen    Min II 13.3.
KN    Cen    B - V: +1.36, +1.75. [A/H] = 0.2.
KQ    Cen    Alternating periods 136d, 159d.
KT    Cen    B - V: +0.46. Min II 12.72. Min II - Min I = 0.392P
             (JD2441686 - 721); apsidal motion is observed [08094].
KY    Cen    Min II 13.3.
KZ    Cen    B - V: +0.30, +0.72.
LL    Cen    Min II 13.1.
LR    Cen    Min II 12.30.
LT    Cen    Min II 9.6.
LU    Cen    The period may be twice longer.
LV    Cen    B - V: +1.3, +1.7.
LW    Cen    Min II 9.6. In the field of the open cluster IC 2944.
LX    Cen    Min II 13.55.
LZ    Cen    Min II 8.50.
MM    Cen    Min II 12.7.
MN    Cen    Min II 8.7. VB A (B 10.9m, 7", 147deg).
MP    Cen    Min II 10.0.
MQ    Cen    Min II 10.1.
MR    Cen    Min II 10.5.
MV    Cen    Min II 14.6.
MY    Cen    B - V: +1.58, +1.94.
NO    Cen    Min II 14.2.
NP    Cen    Min II 10.2.
NY    Cen    Min II 11.9.
OO    Cen    <B - V> = 1.84.
OP    Cen    Min II 13.8.
OU    Cen    Min II 10.9.
OV    Cen    Min II 11.0.
OX    Cen    Min II 14.3.
QS    Cen    d = 0.03P.
QT    Cen    Min II 13.4.
QY    Cen    <B - V> = 2.16.
QZ    Cen    P var? The shape of the light curve varies?
V0339 Cen    VB A (B ~13m, SP). B - V: +1.08, +1.47.
V0343 Cen    Min II 13.5.
V0344 Cen    Min II 12.3.
V0346 Cen    In the field of the open cluster Stock 14. Min II 8.8.
             Min II = 2421966.835 + 6.32189d*E.
V0348 Cen    d = 0.010P.
V0349 Cen    Min II 14.5.
V0350 Cen    Min II 10.3. Min II = 2430870.192 + 3.216906d*E.
V0351 Cen    Epoch of Min is given.
V0356 Cen    Min II 15.0.
V0358 Cen    Epoch of Min is given.
V0365 Cen    d = 0.040P.
V0373 Cen    VB A (B ~4" np).
V0377 Cen    d = 0.003P.
V0379 Cen    Min II 8.9.
V0380 Cen    Min II 10.0.
V0383 Cen    Min II 13.6:, Min II - Min I = 0.609P.
V0384 Cen    Min II 12.2. DII = 0.062P. Min II - Min I = 0.667P.
V0385 Cen    Min II 13.0.
V0388 Cen    Min II 15.7.
V0399 Cen    d = 0.020P. Min II 13.1.
V0405 Cen    P var, 30d - 40d.
V0412 Cen    VB A (B 59", 266deg).
V0419 Cen    P var. Max = 2428099.25 + 5.50713d*E (JD2428099 - 33573);
             since JD2434900 - see Table.
V0420 Cen    B - V: +0.45, +0.97. P var. Nonlinear term:
             -0.000090d*E**2.
V0427 Cen    Epoch of Min is given.
V0436 Cen    SB (P = 0.0669d). Photometric P during supermaxima
             0.06383d [08838]. Rapid oscillations in supermaxima
             Delta(m) ~0.002m, P ~19.6s [08049].
V0440 Cen    d = 0.033P. Min II is possible.
V0443 Cen    d = 0.025P.
V0491 Cen    Very flat minima; close companion?
V0495 Cen    d = 0.042P. Min II 10.6. Min II - Min I = 0.520P.
V0496 Cen    Possible member of the open cluster NGC 4755.
             B - V: +1.02, +1.33.
V0498 Cen    P may be twice shorter.
V0499 Cen    (k - b)2 = 0.23.
V0504 Cen    Semiregular  variations (P1 ~130d, P2 ~411d)
             are also observed [08836].
V0506 Cen    The chart in [06286] is wrong.
V0508 Cen    Min II 13.2.
V0526 Cen    Delta(m) var. P var. Max = 2425707.540 + 0.56153d*E
             (1929 - 1930); during 1931 - 1940 - see Table.
V0527 Cen    The chart in [06286] is wrong.
V0532 Cen    Star 1 [09078]. X-ray source 3A 1431-409.
V0544 Cen    2AS E 1440-39? [05962]. The chart in [06286] is wrong.
V0545 Cen    Magnitude in Max var (12.6 - 14.5), P = 1800d?
V0553 Cen    [Fe/H] = -0.1; [C/Fe] = +0.8.
V0565 Cen    Min II 13.9. Type RR is not excluded (P = 0.238072d).
V0574 Cen    sp star of a pair.
V0577 Cen    According to improved coordinates, the star is actually in
             Hydra.
V0585 Cen    Min II 13.0.
V0592 Cen    Mean brightness var.
V0593 Cen    Possible member of the open cluster Stock 16. Min II 11.2.
V0594 Cen    V133 (omega Cen); non-member of the cluster. Min II 14.4.
V0606 Cen    Min II 9.8.
V0607 Cen    Min II 14.1.
V0608 Cen    Min II 13.1.
V0609 Cen    Min II 13.6.
V0615 Cen    Min II 14.0.
V0617 Cen    Min II 13.8:.
V0619 Cen    In the field of the open cluster NGC 5316.
V0621 Cen    d = 0.05P.
V0624 Cen    Min II 14.9.
V0625 Cen    Min II 15.0.
V0627 Cen    d = 0.02P.
V0628 Cen    Min II 13.2.
V0630 Cen    Min II 14.2. d = 0.06P.
V0635 Cen    Min II 13.9.
V0636 Cen    Min II 8.8.
V0644 Cen    During the faint phase in 1951 the shell spectrum was
             observed [02128]. Type E with a very long period is
             possible [06763].
V0645 Cen    Proxima Cen = alpha Cen C. mu = 3.809", P = 281.7deg.
             Soft X-ray source.
V0646 Cen    d = 0.022P. Min II 9.1.
V0662 Cen    P ~2.48d or 2.95d.
V0672 Cen    Min II 11.4 - 11.6 (var).
V0673 Cen    Depth of Min II 0.05m.
V0674 Cen    Blazhko effect: Pi = 29.5d. 0.15P <= M - m <= 0.23P.
V0676 Cen    Min II 12.5.
V0677 Cen    Min II 11.6.
V0678 Cen    Min II 10.6.
V0679 Cen    9.8"p, 1.1"n from CPD -62deg 2167.
             The star is at the edge of a dark cloud in a bright nebula,
             a part of IC 2944, in the field of a very poor open
             cluster. Since 1950 till 1954 faded by 2.5m. Rather red.
             "Screening" by the edge of a dark nebula?
V0682 Cen    IR excess.
V0684 Cen    Depth of Min II 0.05m.
V0685 Cen    Min II 9.5.
V0686 Cen    RV type is not excluded.
V0687 Cen    Min II 14.1. DII = 0.12P. Min II - Min I = 0.580P.
V0688 Cen    Min II 12.7.
V0689 Cen    Min II 12.1.
V0690 Cen    Depth of Min II 0.03m.
V0692 Cen    Min II 11.6. Min II - Min I = 0.481P.
V0701 Cen    VB? d = 0.026P. Min II 9.1.
V0704 Cen    IR excess.
V0716 Cen    Min II 6.21.
V0742 Cen    Min II 10.1.
V0743 Cen    (k - b)2 = 0.20. Elements almost as well satisfactory:
             Max = 2439243.6465 + 0.10222560d*E.
V0745 Cen    Min II 9.6.
V0746 Cen    = V467 Cen. Marked as V467 Cen in the chart.
V0747 Cen    Min II 10.05.
V0748 Cen    B - V: +0.31, +1.21; U - B: -0.66, -0.21. d = 0.106P.
             Narrow Halpha emission. Outside eclipses shows variations
             by 0.05m - 0.1m during several days or several weeks
             (probably irregularly) [06968].
V0752 Cen    Min II 9.61. dI = dII = 0.047P.
V0753 Cen    (k - b)2 = 0.20. In the field of the open cluster NGC 3960;
             probably non-member. Type DSCT is possible.
V0754 Cen    Slight Min II.
V0755 Cen    In the Coalsack.
V0756 Cen    In the Coalsack. High excitation lines (OVII, OVIII, CV)
             are present in the spectrum. WR type is possible [07372].
V0757 Cen    Min II 8.6.
V0758 Cen    d = 0.07P. Min II 9.15.
V0759 Cen    Min II 7.56.
V0761 Cen    IR excess.
V0763 Cen    VB A (B 13m, 7", 163deg).
V0766 Cen    VB A (B 10.01m, B0Ibp, 9", 318deg). IR excess.
V0767 Cen    VB A (B 11.52m, 21", 350deg).
V0768 Cen    Possible P: 60d - 80d.
V0770 Cen    According to [07570], const?
V0772 Cen    In the region of the open cluster IC 2944.
V0775 Cen    EB type is possible. Deep Min II.
V0777 Cen    Deep Min II.
V0779 Cen    Cen X-3 (3U 1118-60). <B - V>: +1.04; <U - B>:  -0.08.
             Min II 13.39. Porb var. The shape of the light curve
             varies. Epoch of Min I is given. Epochs of Min II coincide
             with the moments of X-ray eclipses. X-ray pulses are
             observed with Ppuls = 4.834477s (epoch JD2442785.3);
             Ppuls decreases [07612]. No rapid optical oscillations
             were found.
V0783 Cen    B - V: +0.35.
V0784 Cen    Very red.
V0788 Cen    Min II 5.90.
V0790 Cen    VB B (A 4.52m; 60", 343deg).
V0791 Cen    In the region of globular cluster omega Cen (NGC 5139).
             Cluster non-member.
V0795 Cen    VB A (B 12.29m, 33.9", 170deg; C 12.79m, 36", 220deg).
V0801 Cen    4U 1145 - 61 = 2S 1145 - 619. Primary component has a low
             density envelope expanding with the velocity of 1800 km/s.
             V sin i = 290 km/s. X-ray pulsar (P = 291.8s
             [08883]). Max (X) = 2442519.5 + 187.5d*E [08881].
V0803 Cen    Extremely hot hydrogen-deficient helium star.
V0807 Cen    VB (9.9m, 10.1m, 0.4", 258deg, 1931).
             It is not known which of the components varies.
V0810 Cen    Member of the cluster Stock 14.
V0813 Cen    In the region of globular cluster omega Cen (NGC 5139).
             V65 (NGC 5139).
V0814 Cen    In the region of globular cluster omega Cen (NGC 5139).
             V78 (NGC 5139). Min II 14.165:. Primary
             component is probably intrinsically variable [08884].
V0816 Cen    Primary oscillation is superimposed by the oscillations
             with freguencies: F2 = 4.9229, F3 = 4.7343, F4 = 4.9317
             [02591].
V0820 Cen    [Fe/H] = -2.5; Vr = +260 km/s.
V0822 Cen    Cen X-4.
V0825 Cen    In the region of globular cluster omega Cen (NGC 5139).
             Cluster non-member. V2 (NGC 5139).
V0826 Cen    In the region of globular cluster omega Cen (NGC 5139).
             Cluster non-member. V129 (NGC 5139).
V0902 Cen    VB, rho = 12". Variability may be spurious.
V0915 Cen    The variability type is not quite consistent with the spectral
             type (B9II/III).
V0921 Cen    High proper motion (LTT 4397) not confirmed by HIPPARCOS data.
V0933 Cen    HIPPARCOS data contradict the luminosity class V.
V1015 Cen    Variability type and luminosity class (III) do not agree.
V1045 Cen    Background field star.
bet   Cen    VB A (B 4.1m, 1.3", 251deg, 1960). SB1 (P = 352d
             [08887]. Multiperiodicity; sometimes brightness is constant
             [08215]. Soft X-ray source.
del   Cen    VB A (B 4.8m, 68.6", 325deg; C 6.5m, 16.6", 227deg).
eps   Cen    VB A (B 13.0m, 36.0", 158deg). There is a secondary light
             oscillation with the amplitude of 0.0034m and elements:
             Max = 2441041.058 + 0.17696d*E.
eta   Cen    VB A (B 13.5m, 5.6", 270deg, 1897); SB?
mu    Cen    VB A (B 13.63m, 48", 128deg).
omi 1 Cen    VB A (B 11.4m, 13.5", 125deg).
T     Cep    P var. Max = 2414252 + 386.05d*E (JD2406900 - 20490);
             Max = 2431086 + 394.93d*E (JD2420490 - 32900);
             Max = 2440262 + 379.22d*E (JD2432900 - 42200); since
             JD2442200 Max = 2444171 + 392.7d*E. Mean value of the
             period is given in the Table. SiO maser.
U     Cep    VB A (B 11.83m, 13.9", 62deg; C 12.3m, 23.0", 318deg).
             0.010P <= d <= 0.040P. Min II 6.93. P var. Min I =
             2407890.3346 + 2.4928551d*E + 5.15d*10**(-9)*E**2
             (JD2388855 - 2440790) [06468]; analysis of period
             variations in this interval see also in [07395];
             Min I = 2441395.3604 + 2.4931048d*E (JD2440790 - 41600);
             Min I = 2441679.5716 + 2.4930432d*E (JD2441600 - 950);
             Min I = 2443753.7982 + 2.4930679d*E (JD2442100 - 43800);
             since JD2444000 - see Table. Shape of the light curve
             and depth of minima vary. Brightness of the secondary (G8)
             varies sporadically. Subgiant brightening accompanies
             eruptive mass transfer. The gaseous stream moving to the
             primary (B7) component forms around it gaseous ring or
             disc [08889].
W     Cep    Slow oscillations with Pi ~2000d are superimposed by
             oscillations with P ~350d.
X     Cep    OH emission?
RS    Cep    d = 0.039P. P var. Min = 2417140.469 + 12.419925d*E
             (JD2410000 - 31000) [02431]; since JD2431000 - see Table.
RZ    Cep    P var. Max = 2411640.654 + 0.308697d*E
             (JD2411640 - 15000); Max = 2417144.620 + 0.3086203d*E
             (JD2415600 - 20200); Max = 2421175.611 +
             0.3086699d*E (JD2421175 - 23000); Max =
             2423768.475 + 0.3086918d*E (JD2423000 - 31700);
             Max = 2433768.493 + 0.3086383d*E (JD2433700 -
             38300) [08890]; Max = 2438207.938 + 0.308645d*E
             (JD2438200 - 39040) [03879]; Max = 2440834.579 +
             0.3086735d*E (JD2440800 - 42640) [08890];
             since JD2442640 - see Table. Shape of the light curve and
             the amplitude A vary with the Blazhko effect period
             Pb = 96.8*P0 = 29.88d; Min A = 2441464.147 + 29.88d*N
             [08891]. Long period variation of P0 with a period ~50
             years is possible. Delta(S) = 6.
SS    Cep    Mean brightness varies with cycles from some hundreds to
             thousands days.
SU    Cep    Min II 10.6.
SV    Cep    IR excess.
SX    Cep    In the region of the nebula NGC 7023.
SY    Cep    Min II 12.70. P var?
SZ    Cep    VB A (B 12.3m, 24.9", 263deg). S4/6e.
TT    Cep    VB A (B 17.0m, 8", 160deg).
TY    Cep    Epoch of Min I is given.
UZ    Cep    P var. Max = 2440969 + 297.68d*E (JD2414000 - 42000);
             since JD2440000 - see Table.
VV    Cep    VB (0.05", 174deg, 1950)? 0.066P <= D <= 0.091P;
             0.040P <= d <= 0.077P. Depth of eclipses: 2.30m (lambda
             3500 A), 1.9m (U), 0.4m (B). M-component is of SRC type:
             Max = 2443045 + 118.37d*E [08698, 08894]; A(V) <= 0.33m.
             Light oscillations are also noted with P ~58d [08895],
             25d and 150d [08896]. B-component may be also an intrinsic
             variable [02416]. Gaseous streams. Strong variable magnetic
             field.
VW    Cep    VB A (B 10.3m, a = 0.51", P = 30.45a [08897]); mu alpha =
             +0.0899s, mu delta = +0.560". Min II 7.56.
             Shape of the light curve and depths of Min I and Min II
             vary. P var. Min I = 2433483.4257 + 0.27831758d*E +
             0.050d*cos(0.004813deg*(E - 4700)) (JD2424763 - 41200)
             [06483]; since JD2441000 - see Table. Period
             change study see also in [08899]. X-ray source.
VZ    Cep    Min II 9.93.
WX    Cep    Min II 9.14; dI = 0.01P, dII = 0.00P.
WY    Cep    Min II 11.5. P var [02545].
WZ    Cep    Min II 11.9.
XX    Cep    Min II 9.26. P var. Min I = 2425096.449 + 2.337340d*E
             (JD2414930 - 30000); Min I = 2441539.4917 + 2.3373059d*E
             (JD2430000 - 42300) [08902]. Since JD2441500 - see Table.
XY    Cep    Min II 10.10. P var?
XZ    Cep    Min II 8.43.
ZZ    Cep    VB A (B 10.2m, A2 P, 3.6", 202deg; C 10.87m, A5V,
             20.6", 219deg). Min II 8.74.
AH    Cep    Min II 7.03. Depth of minima varies. P var.
             Min I = 2434989.3702 + 1.7747274d*E (JD2415500 - 35000)
             [03604]; since  JD2434900 - see Table: +3.12d*10**(-9)*E**2.
AI    Cep    Min II 9.48.
AN    Cep    Since JD2425200 primary and secondary maxima and minima
             appeared, and mean cycle became 254d.
AV    Cep    d <= 0.04P.
BB    Cep    d = 0.050P.
BE    Cep    Min II 13.0.
BF    Cep    P var. Max = 2437236 + 426.11d*E (JD2423600 - 37300);
             Max = 2441665 + 442.3d*E (JD2437300 - 42500); since
             JD2442500 - see Table.
BH    Cep    Sometimes strong Algol-like light weakenings are observed.
BO    Cep    Sometimes strong Algol-like light weakenings are observed.
CO    Cep    Min II 12.6; Min II - Min I = 0.552P; DII = 0.080P.
CP    Cep    P var?
CQ    Cep    Shape of the light curve and depth of minima vary.
             According to [07401] on 1969 March 28/29 on the phase
             0.56P a light decrease by 0.1m was observed and then a
             rapid flare by 0.35m U, 0.13m B, 0.14m V. P var. Nonlinear
             term: -10**(-9)*E**2.
CR    Cep    P var. Max = 2436846.94 + 6.23318d*E (JD2415000 - 30000)
             [03157]; since JD2430000 - see Table.
CV    Cep    S7/1.5. Mean brightness varies with a cycle ~2000d [00159].
CW    Cep    VB A (B 12.29m, 20", 310deg). Min II 8.01;
             Min II -  Min I = 0.478P (1972 yr). There is a sinusoidal
             term in the elements: +0.0250d*sin(0.0626deg*E - 28.3deg).
             Apsidal motion with P = 43a.
CX    Cep    Min II 12.16.
CY    Cep    Min II 16.5.
DD    Cep    P var. Max = 2427960 + 167.6d*E (JD2427900 - 30000);
             Max = 2429968 + 173.0d*E (JD2429900 - 33600);
             since JD2433600 - see Table.
DH    Cep    In the region of the cluster NGC 7380. Apsidal motion with
             P = 2.6a [00165].
DK    Cep    Min II 12.4.
DL    Cep    Min II 12.7.
DO    Cep    VB B (A 9.87m, M4V; a = 2,4", P = 44.78a, e = 0.408);
             mu = 0.852", P = 242.6deg.
DP    Cep    Min II 14.4.
DQ    Cep    Multiperiodicity: P0 = 0.12420d: [08137], P1 = 0.061177d
             [08914].
DX    Cep    P var. Max = 2430603.712 + 0.5260395d*E (JD2415700 - 31000)
             [00001]; since JD2431000 - see Table. Delta(S) = 7.
DY    Cep    Min II 11.8.
EE    Cep    A var?
EF    Cep    Min II 12.6. P var?
EG    Cep    Min II 9.61. P var. Min I = 2439774.3322 + 0.54462091d*E
             (JD2415200 - 41000) [00001]; since JD2441000 - see Table.
EH    Cep    In the dark cloud near the diffuse nebula and the cluster
             NGC 7023.
EI    Cep    Min II 7.98.
EK    Cep    Min II 8.06; Min II - Min I = 0.545P (1965). Min II =
             2439022.8484 + 4.427797d*E [08160].
             Apsidal motion (P = 4700a  +- 600a) [08923].
EL    Cep    P var.
EM    Cep    In the region of the cluster NGC 7160. VB A (a 12.8m,
             19.8", 281deg; B 7.9m, 62.5", 146deg). Min II 7.16.
             Shape of the light curve and depth of minima vary.
EO    Cep    Min II 12.3.
EP    Cep    In the cluster NGC 188. Min II 17.0.
EQ    Cep    In the cluster NGC 188. Min II 16.7.
ER    Cep    In the cluster NGC 188. Min II 16.27.
ES    Cep    In the cluster NGC 188. Min II 15.8.
             P var. Min I = 2439082.238 + 0.34468d*E (JD2438480 - 39090);
             Min I = 2439236.501 + 0.34264d*E (JD2439090 - 39280);
             Min I = 2439594.548 + 0.34250d*E (JD2439400 - 39600);
             since JD2439600 - see Table. A var.
EX    Cep    Min II 11.6.
EY    Cep    Min II 10.4.
EZ    Cep    P var. Max = 2416803.627 + 0.378990d*E (JD2415400 - 20000)
             [00001]; since JD2420000 - see Table.
FH    Cep    Min II 12.1.
FL    Cep    d = 0.02P.
FS    Cep    Min II 12.0.
FT    Cep    VB A (B 18.3m, 5", 27deg). In the region of the diffuse
             nebula and the cluster NGC 7023.
FU    Cep    In the region of the diffuse nebula and the cluster
             NGC 7023.
FV    Cep    In the region of the diffuse nebula and the cluster
             NGC 7023. P = 0.4628d.
FW    Cep    In the region of the diffuse nebula and the cluster
             NGC 7023.
GI    Cep    Min II 11.9.
GK    Cep    Min II 7.35; dI = dII = 0.03P; Min II - Min I = 0.502P.
             P var. Min I = 2425189.526 + 0.9361614d*E
             (JD2415000 - 27500); Min I = 2438694.7070 + 0.9361714d*E
             (JD2427500 - 38200) [00001]; since JD2438200 - see Table.
GL    Cep    In the region of the diffuse nebula IC 1396 and the
             cluster Tr 37.
GM    Cep    In the region of the diffuse nebula IC 1396 and the
             cluster Tr 37.
GP    Cep    In the region of the HII zone S 132. Quadruple system,
             consisting of a WN6 + O8-B0III: eclipsing pair
             (P = 6.6883d) physically associated with an O + O pair
             (P = 3.4698d); the latter pair may be also an eclipsing
             or ellipsoidal variable [08931].
GS    Cep    Min II 10.6.
GT    Cep    Min II 8.6.
GW    Cep    Min II 12.00.
HK    Cep    Min II 14.4.
HZ    Cep    In the region of the diffuse nebula and the cluster
             NGC 7023.
IL    Cep    VB A (B 11.91m, 7", 326deg); P = 2.802d?
IM    Cep    Min II 13.6.
IO    Cep    Min II 11.7.
IP    Cep    Min II 12.1.
IR    Cep    VB (Delta(m) ~0.0m, 0.0" -0.2"). P var.
             Max = 2431060.878 + 2.114016d*E (JD2428335 - 31060) [00001];
             since JD2440900 - see Table.
IV    Cep    VB B (A 16m; B 2.1", 191deg).
IW    Cep    Min II 13.7; Min II - Min I = 0.52P.
IX    Cep    d = 0.03P. Min II 17.0.
KL    Cep    d = 0.019P.
KP    Cep    Depth of Min II 0.03m.
KV    Cep    Min II 14.3.
KY    Cep    Flare with 65 sec duration. There is a blue object on the
             place of the flare [00001].
KZ    Cep    VB (8.6m, 8.6m; 1.9", 348deg). Depths of spectral lines
             vary: P = 0.212938d [06488].
LL    Cep    Min II 14.0.
LM    Cep    Min II 12.8.
LP    Cep    Min II 13.8; Min II - Min I = 0.55P.
LQ    Cep    Eastern component of a double star.
LU    Cep    VB.
LW    Cep    Depth of Min II 0.05m.
LZ    Cep    Min II 5.63. In the Table: P(Vr) [04627].
MN    Cep    Depth of Min II 0.08m?
MQ    Cep    Min II 15.7.
MT    Cep    Min II 15.5.
MX    Cep    SB (P = 16.03d) [08947].
MY    Cep    In the cluster NGC 7419. Emission OH, H2O.
MZ    Cep    In the region of the cluster NGC 7419.
NN    Cep    Min II 8.52.
NR    Cep    Min II 13.6; d = 0.025P?
NS    Cep    Depth of Min II 0.04m.
NW    Cep    Preceding component of a close VB. Min II 10.7.
NY    Cep    VB A (B 10.33m, 10", 190deg); d = 0.003P; SB2, e = 0.49;
             Delta(gamma) = gamma2 - gamma1 = 32 km/s  [07412].
OS    Cep    Very red.
OT    Cep    Min II 13.3.
OZ    Cep    Red.
PS    Cep    In the region of the cluster NGC 7380. SB2 (P = 2.09168d)
             [05479].
PV    Cep    In the dark cloud near the diffuse nebula and the cluster
             NGC 7023. At the apex of the bright variable fan nebula.
PW    Cep    In the region of the diffuse nebular and the cluster
             NGC 7023.
QZ    Cep    The map of surroundings given in [04015] for BV 323 is in
             reality the map for BV 324 = QZ Cep. Min II 11.9.
V0338 Cep    Min II 9.52.
V0342 Cep    B - V = +3.6.
V0344 Cep    B - V = +4.4.
V0345 Cep    B - V = +5.0.
V0346 Cep    B - V = +4.6.
V0347 Cep    B - V = +4.5.
V0351 Cep    VB A (B 13m, 20", 135deg). P var. Max = 2430615.57 +
             2.80511d*E (JD2429160 - 34300); Max = 2435749.12 +
             12.80556d*E (JD2435310 - 40885) [02830]. Since
             JD2442020 - see Table.
V0421 Cep    SB, Porb1 = 5.4136d, Porb2 = 225.44d.
V0447 Cep    The variability may be due to the fainter (B) component.
V0448 Cep    SB, Porb = 7.7320d.
V0453 Cep    SB, Porb = 54.723d.
V0454 Cep    SB, Porb = 5.6556d.
V0711 Cep    Variability refers to combined brightness of two nearly equal
             components at 5" separation.
bet   Cep    VB A (A 6m, 0.204", 47.2deg, 1977.9; B 7.84m, A2V, 13.6",
             250deg). SB1 (Porb = 10.893d) [06486]. P var.
             Max(Vr) = 2417359.715 + 0.1904795d*E (JD2415750 - 22000);
             Max(Vr) = 2422203.790 + 0.1904844d*E +
             2.9440d*10**(-11)*E**2 + 3.2671d*10**(-17)*E**3
             (JD2422000 - 42630) [00177]. Elements given in the Table
             satisfy observations in 1967 - 69.
del   Cep    VB A (B 13.0m, 20.0", 285deg; C 6.10m - 6.37m, B7IV,
             41.0", 191deg. P var. Max = 2393659.856 + 5.366438d*E
             (JD2372200 - 96900); Max = 2413960.73 + 5.366386d*E
             (JD2396900 - 2414050); since JD2414050 - see Table.
             All observations in the interval JD2373090 - 45000 are
             well represented also by the elements with a square term:
             Max = 2442756.490 + 5.366270d*E - 7d*6*10**(-9)*E**2
             [08632].
eps   Cep    VB A (B 9.5m, 127.8", 15deg, 1918).
             Multiperiodicity: P2 = 0.068073d
             (A2/2 = 0.0061m), P3 = 0.011823d? (A3/2 = 0.0022m);
             A1/2 = 0.0079m.
zet   Cep    Radial velocity varies.
mu    Cep    VB A (B 12.3m, 19.4", 262deg; C 12.7m, 41", 299deg).
             There is also the cycle with 4400d duration [08957].
W     Cet    S5.5/2e.
RR    Cet    [Fe/H] = -1.26. P var. During JD2417500 - 28820
             Max = 2417501.444 + 0.55302577d*E; since JD2433180 - see
             Table. According to [08726], the graph of O - C deviations
             from the elements given in [03506] is approximately
             sinusoidal, with Pi = 2600d and the amplitude 0.025d.
RU    Cet    (k - b)2 = 0.01. Delta(m) var? P var [02455]. Max =
             2426964.019 + 0.5863003d*E (JD2426500 - 28430)
             [00181]; Max = 2434143.056 + 0.5862676d*E
             (JD2433100 - 35820) [02431]; since JD2435820 - see Table.
RV    Cet    Delta(S) = 9.
RW    Cet    Min II 10.5. P var. During JD2426500 - 41000
             Max = 2426585.503 + 0.9751814d*E [00001]; since
             JD2441000 - see Table.
RX    Cet    Delta(S) = 5. P var. Before JD2428500 Max =
             2425938.271 + 0.5737100d*E [03506]; since
             JD2430000 - see Table.
RZ    Cet    Delta(S) = 6.7. P var. During JD2426585 - 28630
             Max = 2426585.448 + 0.510633d*E [03506]; current
             elements - see Table.
SS    Cet    d = 0.025P. P var. Min = 2429321.250 + 2.9739509d*E
             (JD2427340 - 30700) [02419]; Min = 2430698.160 +
             2.973992d*E (JD2429300 - 36650) [03115];
             since JD2440000 - see Table.
SV    Cet    Min II 14.9.
TT    Cet    Min II 11.1.
TU    Cet    D = 0.043P. Min II 10.9. Min II - Min I = 0.478P.
             According to [03564], the spectrum is K2.
TV    Cet    Min II 9.10. DII = 0.03P. Min II - Min I = 0.494P.
TW    Cet    Min II 11.14. P var. Min I = 2430965.595 +
             0.316852d*E (JD2427650 - 31000) [00192]; Min I =
             2433611.3121 + 0.316846d*E (JD2433530 - 615)
             [00001]; since JD2440000 - see Table.
TX    Cet    B - V: +0.34, +0.37. Min II 11.12.
TY    Cet    Min II 12.1.
UU    Cet    (k - b)2 = 0.08. P var. Blazhko effect?
UV    Cet    VB B (A 12.45m, dM5.5e; a = 2.1", P = 25a).
VV    Cet    Min II 11.0. EB type is also possible. RR type with twice
             shorter period is not excluded.
VX    Cet    d = 0.026P.
VY    Cet    Min II 11.70.
VZ    Cet    ADS 1778 B (B 0.61", 122deg; A = omicron Cet).
             Small variations are also observed on the time scale of
             several hours, with superimposed 10 - 15 minute variations
             and rare flares of approximately 2 minute duration
             [06492]. A possible white dwarf with an accretion
             disc [08926].
WW    Cet    VR var (P = 0.160d) [04712].
             Rapid oscillations (~10 min) of brightness are observed
             [04709].
WZ    Cet    Min II 11.0.
XY    Cet    d = 0.02P. Min II 9.34.
YY    Cet    Min II 9.2.
ZZ    Cet    4 stable oscillations are observed simultaneously:
             P1 = 213.132605s, P2 = 212.768427s, P3 = 274.250814s,
             P4 = 274.774562s.
AA    Cet    ADS 1581 A (B 7.7m vis, SB 2, F5, 8.5", 304deg).
             Min II 6.7:. dII = 0.065P.
AB    Cet    ADS 1849 A (B 9.30m, 12", 293deg). SB? (VR var,
             P = 2.997814d). The period of magnetic variations is
             15.9d [08932].
AD    Cet    ADS 180 A (B 10m, 3", 4deg).
CL    Cet    Type ELL: is also possible.
EE    Cet    The variability may be due to the fainter (B) component.
EL    Cet    SB2.
del   Cet    Nonlinear term: +2.20d*10**(-11)*E**2.
omi   Cet    ADS 1778 A (B = VZ Cet, 0.61", 122deg). Maser
             SiO, OH, H2O.
S     Cha    VB A (B 9.29m, 23", 134deg).
T     Cha    Occasionally quasiperiodic light changes are observed with
             periods 3.2323d, 3.4375d, 4.1800d, 3.2436d operating
             during 6 - 26 cycles. IR excess.
Z     Cha    VB A (B 5.6"). Eclipses: Min =
             2440264.68232 + 0.0744992195d*E + 7.88d*10**(-13)*E**2
             [08938]. D = 0.065P; d = 0.026P. Depth of Min:
             1.73m - 2.11m B before the eclipse; 1.38m - 1.97m B after
             the eclipse. Periodic variations during Min light [07000].
             Variations with P = 27.7s during a supermaximum [08049].
RS    Cha    EA/DM. Min II 6.53. One of the components is a pulsating
             variable of DSCT type. P is in the range from 0.074d
             to 0.097d [08403]. Delta(M) = 0.01m - 0.03m in the combined
             light.
RW    Cha    Min II 14.6.
RY    Cha    Min II 14.0.
RZ    Cha    Min II 8.8. DII = 0.11P.
SY    Cha    Quasiperiodic variations were observed. (P = 6.2d [04305],
             P = 7.6d [08946]).
TW    Cha    Quasiperiodic variations (P = 8.68d [04462]).
VW    Cha    IR excess.
VZ    Cha    Quasiperiodic variations (P = 7.27d).
YZ    Cha    Delta(m) (Min II) = 0.4m.
CG    Cha    Min II 14.4.
CH    Cha    Min II 15.1.
CX    Cha    Min II 15.5. Uncertain elements.
CY    Cha    Min II 14.0.
CZ    Cha    Min II 14.6.
DD    Cha    Min II 14.7.
DG    Cha    Min II 14.5.
zet   Cha    SB.
S     Cir    Min II 10.9.
T     Cir    Min II 9.4.
U     Cir    P var. Before JD2417000 Max = 2412560 + 151d*E.
V     Cir    Min II 11.0. According to [00210], varies in the range
             10.8m - 13.0m pg.
W     Cir    Found in Lupus, in 4deg to the north from the position
             published by the discoverer [00211].
TW    Cir    Min II 13.3.
UY    Cir    Red.
UZ    Cir    Epoch of main Max is given. Resembles R Cen.
             Max I - Max II = 160d.
VX    Cir    P var. Before JD2418000 Max = 2414360 + 427d*E.
AQ    Cir    Possibly EW type with twice longer period.
AR    Cir    The magnitude in Min light possibly corresponds to an
             unresolved companion.
AT    Cir    d = 0.02d:.
AX    Cir    SB. VB? (6.5m; 6.5m; 0.5", 143deg, 1913).
BD    Cir    Min II 9.5.
BF    Cir    Min II 8.9.
BG    Cir    Min II 10.3.
BN    Cir    Deep Min II. Twice shorter period is not excluded.
BR    Cir    Cir X-1. According to [08951], the object does not coincide
             with the star (B = 22.5m) labelled as L in the chart in
             [02911] but is situated in ~1" to the south of it and has
             M > 23.5m on IIIa-J plates. Gradual increase of X-ray
             intensity is periodically stopped by an abrupt intensity
             fall. The moments of such transitions T are represented by
             the elements T = 2443292.118 + 16.595d*E [02926]. The X-ray
             intensity falls are accompanied by IR and radio bursts.
             Vr (e alpha) = +250 km/s. In 25' from the supernova
             remnant G 321.9-0.3.
tet   Cir    VB (6.2m, 6.2m, 0.1", 96deg).
T     Col    SiO maser.
U     Col    Min II 10.5.
Y     Col    V2 (NGC 1851).
Z     Col    V1 (NGC 1851).
RS    Col    Min II 9.97. dII = 0.021P.
RY    Col    (k - b)2 = 0.10. P var; nonlinear term: -3.38*10**(9)E**2.
RZ    Col    Min II 11.20.
VW    Col    Variability may be due to component B.
TV    Col    2A 0526 - 328. VB A (B 15.79m, 10", 330deg). Epoch of Max
             of short-term photometric variations is given. The
             following elements describe, respectively, moments of Max
             Vr for Balmer lines and moments of Max for the
             comparatively long-term photometric variations which are
             due to the beat phenomenon for the photometric and
             spectral periods: Max Vr = 2444227.631 + 0.228600d*E;
             Max = 2444191.5 + 4.024d*E. Flickering up to 0.15m B and
             flares up to 0.3m U are also observed [08960].
R     Com    OH emission.
S     Com    Delta(S) = 8.
T     Com    OH, H2O emission.
U     Com    Delta(S) = 5.
V     Com    P var. Max = 2424518.219 + 0.46913844d*E
             (JD2420900 - 26900) [00218]; since JD2438100 - see Table.
             Delta(S) = 8.
W     Com    Radio source ON 231.
X     Com    Z = 0.092. Spectrum description [07415, 08966].
Y     Com    In the region of the globular cluster M 53 (NGC 5024).
Z     Com    In the region of the globular cluster M 53 (NGC 5024).
RR    Com    In the region of the globular cluster M 53 (NGC 5024).
RS    Com    In the region of the globular cluster NGC 5053.
RT    Com    In the region of the globular cluster NGC 5053. A var;
             P var. Max = 2423113.496 + 0.5651925d*E (JD2422700 -
             26450) [00222]; since JD2438535 - see Table.
RU    Com    In the region of the globular cluster M 53 (NGC 5024).
RV    Com    In the region of the globular cluster M 53 (NGC 5024).
RW    Com    In the region of the Comae Berenices cluster. dI = 0.04P;
             Min II 11.56. P var.
             Min I = 2433040.406 + 0.23734705d*E (JD2419680 - 34550)
             [00185]; since JD2439600 - see Table.
RY    Com    P var. Max = 2425007.450 + 0.46894835d*E (JD2425000 -
             27500) [03506]; Max = 2432674.390 + 0.4689397d*E
             (JD2432600 - 38110) [03415]; since JD2438100 - see Table.
             (k - b)2 = 0.07.
RZ    Com    Possible member of the Comae Berenices cluster. Min II
             11.09; dI = 0.043P, dII = 0.039P. P var.
             Min I = 2433396.737 + 0.33850556d*E (JD2425000 - 33300)
             [00226]; since JD2433300 - see Table.
             Shape of the light curve varies.
SS    Com    Min II 11.9.
ST    Com    Delta(S) = 10.
SX    Com    In the region of the globular cluster NGC 4147.
SZ    Com    In the region of the globular cluster NGC 4147.
TU    Com    Shape of the light curve, A and P vary. Mean elements
             are given in the Table. Possible period of Blazhko effect
             is 75d [03584]. [Fe/H] = -1.43.
UU    Com    Member of the Comae Berenices cluster. Light variations
             are due to rotation and pulsations of the star. Rotational
             period is 2.1953d or 1.0256d or 0.9178d. Period of
             pulsations is 0.0227d (A ~0.01m). According to [07985]
             there are two periods of pulsations: P1 = 0.0274d and
             P2 = 0.0209d
             (P2/P1 = 0.76).
UV    Com    [Fe/H] = -1.44.
UW    Com    [Fe/H] = -1.22.
UX    Com    Min II 10.13. P var; nonlinear term: -3.75d*10**(-8)*E**2.
UY    Com    [Fe/H] = -1.51.
UZ    Com    [Fe/H] = -1.44.
VV    Com    [Fe/H] = -1.53.
VW    Com    VB (12.00m, dM 3.5e; 12.3m, dM 4e, 3.0", 23deg, 1945).
             Range of total brightness variation
             is given. According to [08363] the component B is
             variable. However both components may be variables.
VY    Com    Min II 14.5.
AI    Com    Member of the Comae Berenices cluster. VB A (B 6.63m,
             145", 251deg). Pulsations are possible: P = 0.052d
             (A = 0.02m) [08975].
AL    Com    Within 8' to the south-east from the nucleus of M 88
             (NGC 4501) galaxy.
AQ    Com    Min II 15.7.
BM    Com    Min II 13.8.
BS    Com    P var. Max = 2434453.31 + 0.36341d*E (JD2434130 - 35230);
             since JD2435590 - see Table. Shape of the light curve
             varies.
BZ    Com    [Fe/H] = -1.21.
CC    Com    In the region of the Comae Berenices cluster. Min II
             12.09; dI = 0.03P.
CD    Com    [Fe/H] = -1.78.
CF    Com    Shape of the light curve varies.
CG    Com    [Fe/H] = -1.06.
CI    Com    RRC?
CK    Com    P var. Max = 2437370.71 + 0.6940159d*E (JD2437370 - 40130);
             Max = 2441630.35 + 0.6939080d*E (JD2440130 - 41630);
             since JD2441630 - see Table. Blazhko effect.
             [Fe/H] = -1.68.
CL    Com    [Fe/H] = -1.00.
CN    Com    Min II 13.5.
CP    Com    [Fe/H] = -1.19.
CT    Com    In the region of the Comae Berenices cluster.
CV    Com    In the region of the Comae Berenices cluster.
CX    Com    In the region of the Comae Berenices cluster. Not member
             of the cluster.
DD    Com    Min II 14.90.
DG    Com    Min II 14.6.
DL    Com    P var?
DR    Com    EW? P = 0.45184d?
DS    Com    [Fe/H] = -1.32.
DT    Com    [Fe/H] = -1.60.
DU    Com    [Fe/H] = -1.45.
DV    Com    [Fe/H] = -1.57.
DW    Com    [Fe/H] = -1.53.
EE    Com    P = 0.539533d also satisfies observations. [Fe/H] = -1.64.
EF    Com    [Fe/H] = -1.90.
EG    Com    [Fe/H] = -1.29.
EI    Com    [Fe/H] = -1.68.
EL    Com    P = 0.52362d also satisfies observations.
EM    Com    [Fe/H] = -1.64.
EN    Com    [Fe/H] = -1.19.
EO    Com    [Fe/H] = -1.51.
EP    Com    [Fe/H] = -0.98.
EQ    Com    Min II 15.3.
ER    Com    [Fe/H] = -1.51.
ES    Com    [Fe/H] = -2.02.
EW    Com    [Fe/H] = -1.77.
EX    Com    P = 0.558359d? [Fe/H] = -1.48.
EY    Com    Min II 18.0.
EZ    Com    P = 0.568349d? [Fe/H] = -1.16.
FG    Com    P = 0.3098d also satisfies observations.
FK    Com    Wide emission lines, Halpha and H, K CaII, of variable
             intensity. Epoch of light minimum is given.
FM    Com    The member of the Comae Berenices cluster. Multiperiodicity.
             Cycle of 0.0713d was observed also [08989].
FO    Com    In the region of the Comae Berenices cluster.
FP    Com    In the region of the Comae Berenices cluster. mu = 0.23",
             P = 158deg. Red.
FZ    Com    P = 4.704864d?
GM    Com    In the region of the Comae Berenices cluster.
GN    Com    Member of the Comae Berenices cluster. P > 1d.
GO    Com    In the region of the Comae Berenices cluster.
GP    Com    mu = 0.38", p = 286deg. SB (Porb = 0.032306d).
             Unique object G 61-29. Consists of two interacting white
             dwarfs. The lower mass star, a helium white dwarf,
             transfers mass to the higher mass star surrounded by an
             accretion disk. Usually flares are being observed with an
             amplitude about 0.2m V, 0.5m U lasting about 20 seconds
             [07417, 08991]. Sometimes periods of photometric activity
             arise when amplitude of light variations reaches 0.6m V
             and sharp passages from maxima to minima are being
             observed; the duration of these minima reaches up to 0.14d
             [07417]. When the star is most active, periodic light
             oscillations appear with P = 105 seconds and amplitude
             0.05m - 0.10m V [07062].
GQ    Com    Z = 0.165. Emission H, [OIII]. Irregular light variations.
             <B - V> = +0.16.
GT    Com    Minor planet (679) Pax.
HH    Com    Epoch of Min in V system is given.
HI    Com    In the region of the Comae Berenices cluster.
HK    Com    In the region of the Comae Berenices cluster.
HM    Com    In the region of the Comae Berenices cluster.
HN    Com    In the region of the Comae Berenices cluster.
HO    Com    In the region of the Comae Berenices cluster.
HP    Com    In the region of the Comae Berenices cluster.
HQ    Com    In the region of the Comae Berenices cluster.
HR    Com    In the region of the Comae Berenices cluster.
HS    Com    In the region of the Comae Berenices cluster.
HT    Com    In the region of the Comae Berenices cluster.
HU    Com    In the region of the Comae Berenices cluster.
HV    Com    In the region of the Comae Berenices cluster.
HW    Com    In the region of the Comae Berenices cluster.
R     CrA    In the head of the bright cometary nebula NGC 6729.
             IR excess.
S     CrA    VB A (B 13.5m, 1", 137deg). IR excess.
T     CrA    In the bright cometary nebula NGC 6729. IR excess.
V     CrA    Quasiperiodic variations (P ~75d, Delta(V) ~ 0.2m - 0.9m).
             IR excess.
RS    CrA    sp of two close stars; each of them or both may be
             identified with CoD -39deg 13082.
RW    CrA    Min II 9.4.
SS    CrA    V1 (NGC 6541).
SV    CrA    The period may be twice shorter.
TY    CrA    VB A (B 13.3m, 4", 138deg; C 58", 24deg).
             In the bright nebula NGC 6726/27. P = 1.92d is not
             excluded, in that case Min II = Min I. On the basis of
             visual observations 8.7 - 12.4 v (presumably "spurious
             variability" due to the difficulties of estimates over
             the bright background of the nebula), and the star
             was classified as INSA.
TZ    CrA    Min II 9.72.
UU    CrA    Min II 11.0.
UX    CrA    The period may be twice shorter.
UY    CrA    P var?
VV    CrA    In the region of the bright nebula NGC 6729. IR excess.
AF    CrA    P var. Before JD2418060 Max = 2413710 + 483d*E; since
             JD2418060 - see Table.
AL    CrA    B - V: +0.65, +1.30. [A/H] = -0.2.
AN    CrA    P var. Nonlinear term: -0.006d*10**(-6)*E**2.
AU    CrA    P var. Nonlinear term: -0.026d*10**(-6)*E**2.
AY    CrA    Min II 15.2.
BG    CrA    Min II 15.1.
BH    CrA    P var. Nonlinear term: -0.023d*10**(-6)*E**2.
CM    CrA    P var. Nonlinear term: -0.007d*10**(-6)*E**2.
CR    CrA    Min II 15.7.
CS    CrA    Min II 15.2.
CY    CrA    P var. Nonlinear term: -0.002d*10**(-6)*E**2.
DG    CrA    In the region of the bright nebula NGC 6729. IR excess.
DL    CrA    Min II 13.6.
DN    CrA    P var. Nonlinear term: +0.006d*10**(-6)*E**2.
DZ    CrA    d = 0.02P.
EE    CrA    <mpg> var, 13.5m - 15.5m, P2 = 3000d - 5000d
             Delta(m) (P1 = 167d) ~1.5m.
EK    CrA    P var. Before JD2422600 Max = 2411870 + 421d*E.
FF    CrA    Before JD2423000 Max = 2411530 + 140.2d*E.
FK    CrA    Min II 14.5.
FS    CrA    Min II 14.5.
FW    CrA    Before JD2416600 Max = 2411190 + 112.2d*E.
GS    CrA    Before JD2422600 Max = 2414070 + 284d*E.
IT    CrA    Min II 13.6.
KM    CrA    The chart in [06286] is wrong.
KQ    CrA    [A/H] = -0.7. B - V: +0.76, +1.23.
KT    CrA    Red.
LU    CrA    P = 182d is possible.
MS    CrA    Yellow.
MT    CrA    Min II 13.1.
NO    CrA    Reddish.
QR    CrA    Reddish.
V0347 CrA    B - V: +0.82, +1.17.
V0350 CrA    Min II 13.4.
V0385 CrA    The period may be spurious.
V0413 CrA    (k - b)2 = 0.11.
V0428 CrA    The period may be twice shorter.
V0449 CrA    [A/H] = -0.3.
V0454 CrA    Min II 10.5.
V0455 CrA    d = 0.05P. Min II 13.7.
V0457 CrA    Epoch of Min is given. EW type is also possible, in that
             case the value of P should be doubled.
V0465 CrA    Min II 14.2.
V0467 CrA    P var?
V0471 CrA    Min II 13.3.
V0478 CrA    Sometimes a cycle 60d - 70d.
V0480 CrA    Min II 13.9.
V0490 CrA    P var? The elements represent the observations of 1944.
V0493 CrA    P var?
V0501 CrA    Min II 13.4. Twice shorter period is possible.
V0503 CrA    d = 0.03P.
V0511 CrA    Twice longer period is possible.
V0512 CrA    P var?
V0513 CrA    Min II 13.2.
V0514 CrA    Min II 14.0.
V0527 CrA    P var.
V0535 CrA    P var.
V0541 CrA    P var?
V0545 CrA    VB. Combined brightness with a faint companion is given.
V0553 CrA    P var?
V0566 CrA    Min II 12.7.
V0568 CrA    Sometimes a cycle 60d - 80d.
V0569 CrA    Min II 13.1. EB type is possible.
V0571 CrA    Min II 14.7.
V0572 CrA    Min II 14.0.
V0577 CrA    Min II 13.2. RR type with twice shorter period is possible.
V0578 CrA    RV type with P = 118d is possible.
V0580 CrA    Min II 14.4.
V0595 CrA    P var.
V0601 CrA    Epoch of min is given.
V0603 CrA    Slightly noticeable Min II at the phase 0.5P.
V0604 CrA    d = 0.03P.
V0607 CrA    Min II 14.3.
V0612 CrA    d = 0.03P.
V0615 CrA    P var?
V0622 CrA    Sometimes 55d - 60d cycles.
V0633 CrA    P var.
V0634 CrA    Min II 13.9.
V0648 CrA    Min II is felt at the phase 0.5P.
V0659 CrA    P = 189.4d is possible.
V0667 CrA    In the region of the bright cometary nebula NGC 6729.
             The spectral type is earlier than K.
V0676 CrA    RR type is possible.
V0686 CrA    Max I 5.34, Min I 5.41, Max II 5.35, Min II 5.40 [08970].
V0691 CrA    4U 1822-37. Emissions CIII/NIII lambda 4640 - 50,
             He II lambda 4686, CIV lambda 1550 etc.
V0692 CrA    P = 0.83d is possible.
eps   CrA    Min II 4.95.
R     CrB    IR excess.
S     CrB    OH, H2O, SiO maser.
T     CrB    VB? A (B <= 12m, 0.2"). SB (P = 227.6d).
             The spectral period is present in the photometric data of
             1891 - 1917 and 1960 - 1971 [08978]. The epoch of the first
             outburst JD2402734 (1866). Two smaller outbursts were
             observed in UV light, JD2438030 (1963) and 2442543
             (1975) [08979].
U     CrB    Min II 7.72. P var.
RR    CrB    P2 = 377d. Delta(m) (P1) ~0.5m, Delta(m) (P2) ~0.6m.
RS    CrB    P2 = 69.5d [01100]. Main period oscillation: 9.1m - 11.6m.
RT    CrB    Nonlinear term: +2.01d*10**(-8)*E**2. Min II 10.52 (var).
             DII = 0.09P.
RV    CrB    P var. Max = 2428285.608 + 0.3316217d*E (JD2428285 - 31610);
             Max = 2431705.349 + 0.3317313d*E
             (JD2431705 - 32954); Max = 2433030.572 + 0.331705d*E
             (JD2433030 - 36814) [05496]; Max =
             2440001.453 + 0.331569d*E (1967 - 1971) [06237];
             Max = 2441451.413 + 0.331619d*E (1972 - 1974)
             [07032]. The Table gives current elements. On
             the period changes see also [03506]. Blazhko effect?
RW    CrB    d = 0.028P. Min II 10.29.
TW    CrB    Min II 11.0.
TZ    CrB    ADS 9979 A (B 6.72m, GIV, 6.6", 233deg, 1980).
             SB2 (P = 1.139789d).
             Epoch of Min is given. The variation presented in the
             Table is superimposed by a second one, with the same
             amplitude and P = 0.1d. The amplitude is given
             for the combined light of ADS 9979 A and B, the
             mean magnitude is for ADS 9979 A.
UU    CrB    During JD2444381.73 - .76 a slow flare was observed, with
             maximal amplitude 0.30m in the IK band and 0.18m in the
             U band.
AL    CrB    Spotted rotating G-type giant.
alf   CrB    lambda eff = 7230 A: DI = 0.034P, DII = 0.018P,
             Min II - Min I = 0.66P, depth of Min I 0.10m, Min II
             0.025m.
bet   CrB    VB A (B ~ 5m - 6m, 0.2",  ~130deg, 1978). SB (P = 3833.7d).
             Magnetic field var, P = 18.487d. The epoch of Min light
             is given.
gam   CrB    ADS 9757 (4.2m, 5.6m; A = 0.74", P = 91.0a).
U     Crv    VB A (B 13.5m, 0.4' p).
W     Crv    Min II 11.86. The light curve is asymmetrical, the maxima
             differ in hight by 0.10m.
Y     Crv    Min II 11.7. RRC type with twice shorter period
             is possible.
Z     Crv    d = 0.06P.
RV    Crv    Elements do
             not satisfy some of the published moments of Min.
RZ    Crv    Min II 13.9.
SX    Crv    Min II 9.23. The shape of the light curve varies. Depth of
             Min I 0.20m, depth of Min II 0.18m. In 1972 the system
             became fainter than in 1971 by 0.06m.
TY    Crv    SB2.
R     Crt    Periods of light constancy which last up to 250d occur
             every two or there thousand days. OH, H2O maser.
S     Crt    H2O maser.
T     Crt    Mean light var, P2 = 1006d.
V     Crt    Min II 10.1; Min II - Min I = 0.57P.
W     Crt    (k - b)2 = +0.21.
X     Crt    (k - b)2 = +0.02.
Z     Crt    d = 0.016P.
RR    Crt    P = 293d or 146d is possible.
RV    Crt    Min II 9.4:.
SU    Crt    [Fe/H] > -0.3.
SV    Crt    ADS 8115 A (B 11.5m vis, 1", 220deg). SB2 (P = 5.90513d,
             apsidal motion, P ~700a). Epoch of Min I in B light is
             given. Depth of Min II is 0.015m. EuII and SrII in
             emission.
R     Cru    In the region of the open cluster NGC 4349.
T     Cru    In the region of the open cluster NGC 4349.
U     Cru    P var. Max = 2410143 + 351.4d*E (JD2410100 - 14100) [00237];
             since JD2437600 - see Table.
W     Cru    Min II 9.3.
SU    Cru    [A/H] = -0.8.
SV    Cru    In the region  of the open cluster Ruprecht 97.
             Non-member of the cluster.
SW    Cru    VB A (B 14.0m, 12"). (k - b)2 = 0.27.
SY    Cru    d = 0.05P?
TU    Cru    Min II 11.5.
TW    Cru    Min II 12.85:.
TX    Cru    It is not excluded that actually P is much shorter,
             close to 1d, for instance.
TZ    Cru    P = 2.091140d?
UW    Cru    Min II 12.9; Min II - Min I = 0.536P.
UX    Cru    VB A (B 10"). Min II 12.4; Min I - Min II = 0.325P;
             DII = 0.025P.
VY    Cru    Min II 13.5.
VZ    Cru    P = 1.125810d?
WW    Cru    Min II 13.0.
WX    Cru    d = 0.040P. Light variability in maximum is noted.
WY    Cru    VB A. P = 9.013290d?
XX    Cru    P = 3.28566d?
XY    Cru    Min II 11.7.
XZ    Cru    P = 1.6495930d?
YY    Cru    Min II 13.0.
YZ    Cru    Min II 13.1.
ZZ    Cru    Min II 9.8.
AB    Cru    Min II 8.9.
AC    Cru    Min II 12.1.
AD    Cru    VB A (B 14.5m, 10", 270deg). P var. Max = 2434918.160 +
             6.39844d*E (JD2423800 - 35400) [02309];
             since JD2441000 - see Table.
AE    Cru    Depth of Min II 0.03m.
AF    Cru    According to [01122] Algol-type with the elements:
             Min I = 2424988.959 + 1.895669d*E, D = 0.06P.
             This conclusion must be checked. The star deserves careful
             investigation.
AG    Cru    The blue component is possible [09004].
AI    Cru    In the region
             of the open cluster NGC 4103. Min II 9.94.
AQ    Cru    Min II 13.8.
AT    Cru    Min II 12.6.
AW    Cru    Min II 13.9.
AY    Cru    Min II 11.2.
BB    Cru    Min II 14.0.
BC    Cru    Depth of Min II 0.03m.
BD    Cru    Depth of Min II 0.05m.
BF    Cru    Min II 12.3.
BH    Cru    Epoch of Min I is given in the Table. The light
             curve like the light curves of R Cen and R Nor
             has two maxima and two minima of different
             depths. Max I 7.6m (0.22P), Min II 8.0m (0.41P),
             Max II 7.2m (0.53P).
BI    Cru    Spectrum description [04949].
BK    Cru    In Coalsack region.
BM    Cru    In Coalsack region.
BP    Cru    3U 1223-62. A unique X-system. Consists of an X-pulsar
             with pulse period 698s [09018] moving on an excentric
             orbit (E = 0.47) around the ellipsoidal B2 supergiant with
             orbital period of 41.51d. Accretion of the stellar wind
             from the primary star on the pulsar increases during the
             periastron passage. Therefore large X-flares are observed
             with the elements: T (X Max) = 2433158.09 + 41.51d*E.
             Optical flares are possible.
BQ    Cru    B - V: +1.13, +0.88.
BS    Cru    In the open cluster NGC 4755.
BT    Cru    In the open cluster NGC 4755.
BU    Cru    In the open cluster NGC 4755.
BV    Cru    In the open cluster NGC 4755.
BW    Cru    In the open cluster NGC 4755.
DU    Cru    The identification with NSV 06012 (SIMBAD) is wrong.
bet   Cru    VB A (B 11.4m, 44.3", 322deg; C 7.5m, 372", 23deg).
             Interferometric binary. Multiple periods (the total V
             amplitudes of corresponding oscillations are indicated
             in brackets): P0 = 0.2365072d (0.034m), P1 = 0.160466d
             (0.029m), P2 = 0.121383d (0.01m), P02 = 0.249373d
             (0.016m), P13 = 0.24273d (0.024m), P24 = 0.23931d
             (0.028m), P03 = 0.16342d (0.016m), P14 = 0.16171d
             (0.029m).
tet 2 Cru    SB (P = 3.4380d). BCEPS, P > 1h? [08420].
lam   Cru    Type ELL with
             P = 0.7902d is possible. Amplitude and shape of
             the light curve vary. The secondary oscillation
             (A = 0.007m) with the elements Max = 2441779.034 +
             0.1793d*E is possible.
R     Cyg    VB A (B 9.3m, 91", 14deg). S4/6e - S8/6e.
T     Cyg    VB A (B 10.03m, 10.2", 122deg; C 12m, 13.6", 197deg).
U     Cyg    VB A (B 7.8m, 63.5", 51deg). P var. Max = 2406455 +
             461.57d*E (JD2404590 - 13900); Max = 2414827 +
             470.76d*E (JD2413900 - 19940); Max = 2421806 +
             455.95d*E (JD2419940 - 27380); Max = 2427848 +
             472.85d*E (JD2427380 - 35750); since JD2435750 - see Table.
W     Cyg    There is a second oscillation with P = 235.3d.
X     Cyg    P var. Max = 2410190.86 + 16.3841d*E (JD2410100 -
             23370) [09028]; since JD2417000 - see Table.
             There is a square term in the elements given in the Table:
             +1.01d*10**(-7)*E**2. [A/H] = 0.4.
Y     Cyg    Min II 7.75; E = 0.1458. Apsidal motion: P = 47.6 yr.
             There are sinusoidal terms in the elements:
             +0.1391d*sin(0.06256deg*E) - 0.0076d*sin(2*(0.06256deg*E));
             Min II = 2409454.9174 + 2.9963328d*E -
             0.1391d*sin(0.06256deg*E) - 0.0076d*sin(2*(0.06256deg*E)).
Z     Cyg    OH, H2O emission.
RR    Cyg    VB A (B 12.5m, 18.1", 58deg).
RS    Cyg    VB A (B 7.09m, 132", 355deg; C 9.3m, 56", 106deg).
             Epoch of light minimum is given. The shape of the light
             curve strongly varies. Double maxima are sometimes
             observed (Min II at the phase 0.5P).
RU    Cyg    VB A (B 12.40m V, 10", 224deg; C 11.15m V, 19", 29deg).
RV    Cyg    VB A (B 10m, 142", 118deg).
RY    Cyg    In the region of the open cluster NGC 6883.
RZ    Cyg    The shape of the light curve strongly varies. Alternation
             of high and low maxima, as well as of shallow and
             deep minima is observed, as a rule: 9.8m <= Max <= 12.0m.
             11.8m <= Min <= 14.1m.
SS    Cyg    SB2 (P = 0.27512995d [08285]).
             During maxima of brightness there are oscillations of
             light and X-ray flux with amplitudes about 0.002m V
             and periods changing between 7.29s and 10.90s [06102,
             09032].
SU    Cyg    P var. Max = 2421278.503 + 3.845507d*E (JD2414250 -
             29000) [01559]; Max = 2433095.944 + 3.845664d*E
             (JD2429000 - 33150) [00921]; since JD2434500 - see Table.
SV    Cyg    VB A (B 9.5m V, 145", 140deg).
SW    Cyg    Min II 9.30; d(V) = 0.018P; d(U) = 0.00P. P var. Min I =
             2414782.448 + 4.572937d*E (JD2411340 - 16450);
             Min I  = 2418440.758 + 4.5727923d*E (JD2417060 -
             19740) [00063]; Min I = 2421504.489 + 4.572729d*E
             (JD2421470 - 24970); Min I = 2425185.550 + 4.5728386d*E
             (JD2424960 - 29500); Min I = 2433160.669 + 4.5729841d*E
             (JD2433000 - 36800) [09085]; Min I = 2438584.3081 +
             4.57311736d*E (JD2438600 - 40560) [09085];
             since JD2441160 - see Table.
SY    Cyg    d = 0.040P. Possible depth
             of Min II 0.03m.
             P var. Min I = 2411659.568 + 6.00584d*E (JD2411600 -
             17100); Min I = 2420001.571 + 6.005716d*E
             (JD2418760 - 20760) [01961];
             Min I = 2437069.254 + 6.005626d*E
             (JD2432800 - 37070) [05416].
             Mean elements given in the Table represent epochs of
             Min I in the interval JD2414400 - 37070 up to +- 0.07d.
             According to [04248] the apsidal motion with the period ~46
             years is possible.
SZ    Cyg    [A/H] = 0.5. P var [02392].
             Mean elements given in the
             Table represent epochs of Max up to  +- 0.5d. According
             to [09029] "the O - C diagram has a sinusoidal structure
             as is to be expected for a member of a binary system"
             with P orb = 65 years.
TT    Cyg    VB A (B 10.8m V, 70", 213deg; C 11.1m V, 83", 49deg;
             D 10.7m V, 94", 268deg).
TV    Cyg    According to [03663] - spectrum G0.
TX    Cyg    [A/H] = -0.2. P var. Max = 2436793.138 + 14.708157d*E
             (JD2415000 - 37000); since JD2436700 - see Table.
UU    Cyg    VB A (B 10.7m V, 3.6", 351deg).
UV    Cyg    VB A (B 10.8m V, 0.9", 79deg).
UW    Cyg    P var. Min I = 2419624.501 + 3.450797d*E (JD2410000 -
             20750) [00526]; Min I = 2419624.501 + 3.450752d*E
             (JD2419620 - 33000); Min I = 2433848.508 + 3.450740d*E
             (JD2430000 - 41800); since JD2441800 -
             see Table. Possible depth of Min II 0.05m.
UX    Cyg    P var. Max = 2432444 + 560.3d*E (JD2415670 - 32450);
             Max = 2439352 + 578.0d*E (JD2432450 - 40500);
             since JD2437600 - see Table. Sometimes rapid light
             decreases on the ascending branch near Max are observed
             [01563, 01564]. H2O, OH, SiO maser.
UY    Cyg    Delta(S) = 3.8.
UZ    Cyg    VB A (B 10.8m, 28", 130deg). d = 0.032P; Min II 10.31.
VV    Cyg    Min II 13.2. P var? [03665].
VW    Cyg    d = 0.035P; Min II 10.31. P var. Min I = 2417377.123 +
             8.4305260d*E (JD2415660 - 17400); Min I =
             2430444.061 + 8.4302826d*E (JD2417400 - 30450);
             Min I = 2441116.868 + 8.4303917d*E + 4.31d*10**(-8)*E**2
             (JD2430450 - 41120) [07096]; since JD2440350 - see Table.
VX    Cyg    [A/H] = 0.2. P var. There is a square term in the
             elemenmts +8.02d*10**(-7)*E**2.
VZ    Cyg    P var. Max = 2437103.945 + 4.8645598d*E(JD2416000 -
             41000); since JD2434000 - see Table.
WW    Cyg    d = 0.008P; Min II 10.16. P var [06144]. Mean elements:
             Min I = 2416981.299 + 3.3176924d*E (JD2412000 - 31000)
             [00063]; since JD2431000 - see Table.
WZ    Cyg    Min II 10.9.
XX    Cyg    [Fe/H] = -0.49. P var. Max = 2430671.1010 +
             0.134865026*E(2416560 - 30000); since JD2430000 - see
             Table.
XZ    Cyg    [Fe/H] = -1.2. P var. Max = 2417201.241 + 0.4665878*E -
             0.000107d*10**(-6)*E**2 (JD2414000 - 35000) [02550];
             Max = 2438562.796 + 0.466570d*E (JD2434000 - 39800);
             Max = 2440445.789 + 0.466497d*E (JD2439800 - 41000)
             [06237]; Max = 2441453.3856 + 0.4664731d*E
             (JD2441000 - 42500) [07424]; Max = 2443028.641 +
             0.466438d*E (JD2442500 - 43800) [09101]; Max =
             2444142.650 + 0.466649d*E (JD2443800 - 44200)
             [09102]; since JD2444100 - see Table.
             Besides that the star has a strongly
             expressed Blazhko effect; the period of Blazhko effect
             varies, too [07424, 07425]. 0.13P <= M - m <= 0.22P;
             0.90m <= A(B) <= 1.70m, 0.70m <= A(B) <= 1.30m;
             -0.05P < O - C < +0.05;
             Max A = 2417025.5 + 57.401d*E (JD2417000 - 38500);
             Max A = 2438881.7 + 58.387d*E (since JD2438500).[09103].
             After JD2444000
             Blazhko effect period probably decreased to 56.3d [09102].
ZZ    Cyg    VB A (B 12.63m, 8.5", 43deg.
             Total brightness variation range
             is given. Min II 10.78. P var. Min I = 2417442.419 +
             0.6286185d*E (JD2415000 - 25800) [07427];
             since JD2427950 - see Table.
AA    Cyg    S 6/3.
AC    Cyg    H2O maser.
AD    Cyg    S 5/5.
AE    Cyg    d = 0.039P; Depth of Min II 0.06m.
AF    Cyg    Light curve (1914 - 1956) [09104].
             Two more independent oscillations are superimposed:
             P2 = 175.8d, P3 = 941.2d.
AK    Cyg    VB A (B 11.06m, A7, 20", 85deg).
AV    Cyg    P var. Max = 2420451.9 + 87.48d*E (JD2418782 -
             24823); Max = 2427936.3 + 89.73d*E (JD2426326 -
             28745); Max = 2429440.9 + 87.69d*E (JD2428820 -
             31260); Max = 2436413.8 + 89.63d*E (JD2434610 -
             37130); since JD2437450 - see Table.
             0.27P <= M - m <= 0.50P.
AX    Cyg    VB A (B 10.2m, 18", 52deg).
AY    Cyg    In the region of the open cluster Dolidze 2.
BB    Cyg    P var. Max = 2426360 + 265.7d*E (JD2414900 - 26700);
             Max = 2433091 + 258.6d*E (JD2426700 - 35500); Max =
             2438354 + 266.9d*E (JD35500 - 40200) [09106];
             since JD2439200 - see Table.
BF    Cyg    P orb = 750d [05655].
             Irregular light variations and sometimes observed
             brightenings by 2m - 3m are superimposed by semiregular
             oscillations with the cycle 755d [01039, 08044].
BG    Cyg    P var. Max = 2421190 + 290.35d*E (JD2421150 - 29950);
             Max = 2430546 + 307.3d*E (JD2429950 - 30850); Max =
             2432872 + 289.5d*E (JD2430850 - 34920);
             since JD2435100 - see Table.
BI    Cyg    VB A (B 9.4m, 126", 110deg).
BO    Cyg    D = 0.025P; Min II 12.0.
BR    Cyg    D = 0.020P; Min II 9.58.
BS    Cyg    SC 8/8. P var. Max = 2422655 + 420d*E (JD2422600 -
             24750) [01161]; Max = 2425181 + 431.4d*E (JD2424750 -
             26500) [01171]; since JD2437500 - see Table.
BY    Cyg    VB A (B 16m).
BZ    Cyg    [A/H] = 0.1. Double maximum.
CD    Cyg    [A/H] = 0.2. P var.
             There is a square term in the elements:
             +1.54d*10**(-6)*E**2.
CG    Cyg    VB A (B 11.8m, 1.3", 306deg; 1979.7).
             10.10 <= Min II <= 10.44. P var.
             Min I = 2422967.4248 + 0.63114347d*E
             (JD2422900 - 38500); since JD2439000 - see Table. Combined
             light range is given. Shape of the light curve varies
             [08848].
CH    Cyg    Semiregular light variations with the mean cycle 97d;
             mean brightness varies with the cycle ~4700d [01169].
             There are also a cycle 725d [08849], rapid oscillations
             (A <= 0.25m U) and flares [05350]. It is not excluded
             that the system is an eclipsing one [06499].
CI    Cyg    d = 0.084P.
             Depth of eclipses ~0.8m. The eclipses of B star are
             observed. Usually there are light fluctuations near mean
             brightness ( ~12.1m). The outbursts last some dozens
             and hundreds days. Light curves [06155, 08044, 08850,
             08851]. Emissions of H, He I, He II, [O III], and N III.
CM    Cyg    S 4/6.5e.
CU    Cyg    P var. Max = 2422643 + 223.8d*E (JD2422600 - 26500);
             since JD2426500 - see Table.
CV    Cyg    dI = 0.06P; Min II 11.33. P var. Min I = 2424458.348 +
             0.9834523d*E (JD2414300 - 24500); since JD2424450 - see
             Table. Shape of the light curve and Min I depth vary.
CY    Cyg    SC 2/7.5.
CZ    Cyg    P var. Max = 2424500 + 284d*E (JD2424500 - 33600)
             [03122]; since JD2432700 - see Table.
DD    Cyg    P var. Max = 2425465 + 148.30d*E (JD2424800 - 39000)
             [01149]; since JD2439000 - see Table.
DF    Cyg    P var [01177, 06107]. Mean
             brightness varies: Min = 2411292 + 780.2d*E [01571].
DG    Cyg    SiO maser?
DH    Cyg    OH emission?
DK    Cyg    dI = dII = 0.04P; Min II 10.90. P var.
             Shape of the light curve and depth of Min II vary.
DL    Cyg    Min II 9.9.
DM    Cyg    P var. Max = 2425887.560 + 0.4198557d*E (JD2415200 -
             25900) [03506]; Max = 2425887.5597 + 0.41985715d*E
             (JD2425880 - 29250) [00522]; Max = 2433872.420 +
             0.41985842d*E (JD2429250 - 37900) [03506]; Max =
             2438677.708 + 0.4198619d*E (JD2438600 - 41250)
             [07114]; since JD2441240 - see Table.
             There is also Blazhko effect with the elements:
             Max(O - C) = 2442978.97 + 26.01d*E [08853];
             -0.01 d< = O - C <= +0.01d. Delta(S) = 0.
DQ    Cyg    P = 180d?
DT    Cyg    P var. Max = 2424305.651 + 2.49913d*E (JD2424300 -
             28500) [01183]; Max = 2432792.893 + 2.49934d*E
             (JD2430000 - 36000); since JD2436000 - see Table.
DV    Cyg    P var. Max = 2425476 + 146.7d*E (JD2415200 - 29200);
             since JD2432800 - see Table.
DW    Cyg    P var. Max = 2427603 + 279.6d*E (JD2416700 - 33500);
             since JD2433500 - see Table.
DX    Cyg    Min II 14.2; Min II - Min I = 0.515P; DI = 0.22P,
             DII = 0.12P.
DY    Cyg    Slow oscillations are superimposed by rapid ones with
             A = 0.3m [03662]. According to [03148] type EB?
             Min = 2436659.531 + 0.6990d(:)*E (JD2436600 - 37000)
             [03148].
EE    Cyg    Min II 14.5.
EF    Cyg    142d <= P <= 175d.
EH    Cyg    P var. Max = 2427608 + 276.90d*E (JD2416200 - 27610);
             since JD2427800 - see Table.
EI    Cyg    Epoch of Max I is given; heights of Max I and Max II
             differ strongly, the depths of Min I and Min II are almost
             equal. Max I - Min I = 52d.
EK    Cyg    Observations are represented by the elements in the
             interval JD2425200 - 37900 only.
EM    Cyg    Mean cycle varies in the range 19d - 33d [04248, 09111].
             Depth of eclipses 0.25m V; elements of eclipsing system
             light variations: Min = 2437882.8595 + 0.29090950d*E -
             21d*10**(-12)*E**2 [08854].
             Sometimes there are light oscillations with periods
             14.6s - 21.2s and an amplitude up to 0.4% [06102, 09112].
EN    Cyg    d = 0.012P. P var. Min = 2425181.311 + 2.2148998d*E
             (JD2424880 - 29600) [00332]; since JD2433500 - see Table.
ES    Cyg    P var. Max = 2425146 + 157d*E (JD2425000 - 29300)
             [00332]; since JD2432800 - see Table.
EV    Cyg    P var. Max = 2427740 + 259.1d*E (JD2425100 - 29100);
             since JD2433500 - see Table.
             The position of the star in the chart in [00530] is wrong
             [00782].
EZ    Cyg    P var? Shape of the light curve and the amplitude
             strongly vary; 0.40P < = M - m < = 0.48P.
FF    Cyg    S 5.5/6-e.
FG    Cyg    P var. Max = 2426955 + 456.0d*E (JD2416000 - 27000)
             [00001]; Max = 2426955 + 458.8d*E (JD2426900 - 34300)
             [03122]; since JD2439200 - see Table.
FM    Cyg    P var. Max = 2425313 + 274d*E (JD2425300 - 29200)
             [00332]; since JD2429200 - see Table.
FN    Cyg    P var. Max = 2429137 + 314.6d*E (JD2416200 - 29200)
             [00001]; since JD2432800 - see Table.
FO    Cyg    A var. P var. Max = 2425193 + 156.6d*E (JD2425000 -
             29200) [00332]; since JD2432500 - see Table.
FR    Cyg    Min II 14.0; d = 0.03P.
FT    Cyg    P var. Max = 2425184 + 156.7d*E (JD2425100 - 29200)
             [00332]. 83d <= P <= 187d (JD2432500 - 38000).
FY    Cyg    P var. Max = 2425172 + 194.d*E (JD2425100 - 29300)
             [00332]. 130d <= P< = 189d (JD2432500 - 38000).
GG    Cyg    d = 0.079P; Min II 12.1.
GM    Cyg    P var. Min = 2428754.305 + 4.745772d*E (JD2413200 -
             33500) [01209]; since JD2433500 - see Table.
GN    Cyg    P var. Max = 2425448 + 156d*E (JD2425400 - 27400)
             [01155]; since JD2427500 - see Table.
GO    Cyg    Min II 8.73. P var. Intrinsic light variability of the
             components is possible [01210].
GS    Cyg    P = 195d?
GT    Cyg    Depth of Min II 0.05m? P var?
GY    Cyg    Secondary oscillation with P = 4000d and
             A(V) = 0.5m is possible.
GZ    Cyg    Red.
HL    Cyg    d = 0.02P.
HV    Cyg    VB (Northern component).
HY    Cyg    P var. Max = 2425334 + 344d*E (JD2425300 - 29200)
             [00332]; since JD2432760 - LB?
II    Cyg    P var. Max = 2425150 + 82d*E (JD2425120 - 25550),
             Max = 2425475 + 94d*E (JD2425550 - 29250) [00332];
             since JD2432500 77d <= P <= 99d.
IK    Cyg    P var. Max = 2425199 + 77.3d*E (JD2425000 - 29200)
             [00332]; since JD2432500 - see Table.
IT    Cyg    P var. Max = 2425305 + 67.4d*E (JD2425300 - 850)
             [00332]; since JD2432500 - see Table.
IU    Cyg    B - V: +0.90, +1.45. P var. Max = 2429157.6 + 31.22266d*E
             (JD2417800 - 29250); Max = 2433601.3 + 31.1550d*E
             (JD2432700 - 35400); since JD2435400 - see Table.
IV    Cyg    P var. Max = 2425470.406 + 0.33432871d*E (JD2425300 -
             33120) [03506]; Max = 2434122.519 + 0.33433895d*E
             (JD2432700 - 40200) [04248]; since JD2440200 - see Table.
             Shape of the light
             curve varies: 0.10P <= M - m <= 0.20P.
IX    Cyg    P var. Max = 2425173 + 172d*E (JD2425000 - 25900)
             [00332]; since JD2428000 - see Table.
KL    Cyg    P var. Max = 2437906 + 536.8d*E (JD2418500 - 38000)
             [00001]; since JD2438000 - see Table.
KP    Cyg    Delta(S) = 0.
KR    Cyg    Min II 9.37.
KU    Cyg    Min II 11.15; d = 0.047P. Shape of the light curve varies.
KV    Cyg    Min II 11.9.
KY    Cyg    H2O, OH maser.
LN    Cyg    Min II 14.3.
LO    Cyg    Min II 13.3.
LX    Cyg    P var. Max = 2432775 + 460.0d*E (JD2415000 - 33300)
             [01159]; since JD2437900 - see Table. SC 7/9-e - SC 8/8.5e.
MQ    Cyg    VB A (B 17.5m B, 4.5", 122deg). P var. Max = 2432737 +
             428.5d*E (JD2414300 - 33300) [01229]; since
             JD2440000 - see Table.
MR    Cyg    Min II 9.12; d = 0.030P; DII = 0.19P.
MU    Cyg    Min II 14.4.
MY    Cyg    Min II 8.99. Min II - Min I = 0.5021P.
MZ    Cyg    P var. Max = 2427641.914 + 21.162460d*E +
             0.10575d*10**(-3)*E**2 (JD2414900 - 37900) [03689]; since
             JD2443600 - see Table. Probably it is an RV Tau type
             variable, and then the period should be doubled [08862].
             [A/H] = 0.1.
NQ    Cyg    EW type is possible. Close to V736 Cyg.
NU    Cyg    Min II 14.9.
NZ    Cyg    Min II 14.2.
OS    Cyg    P var.
OU    Cyg    Min II 15.6.
OY    Cyg    Star 23 - 30 [01321].
PP    Cyg    Star G in the chart for VV245 [07749].
PR    Cyg    Star 24 - 40 [01321].
PT    Cyg    Star 23 - 55 [01321].
PU    Cyg    Star 25 - 56 [01321].
PX    Cyg    Star 35 - 78 [01321].
PY    Cyg    Min II 15.2.
QS    Cyg    Min II 13.3.
QT    Cyg    Depth of Min II 0.04m.
QU    Cyg    Min II 15.1.
QW    Cyg    Min II 14.1.
QX    Cyg    Min II 14.5.
V0339 Cyg    np component of a close binary.
V0340 Cyg    Min II 14.5.
V0343 Cyg    [A/H] = -0.2.
V0346 Cyg    Companion 13.8m, 0.4' sf. Min II 11.9. P var.
             Min I = 2427270.241 + 2.743345d*E (JD2415000 - 32000);
             since JD2432000 - see Table.
V0348 Cyg    According to [07516] EW type variable with large
             irregularities: Min = 2441567.177 + 0.285768d*E
             (JD2441567 - 95).
V0355 Cyg    Min II 14.3.
V0360 Cyg    P var [06107]. Min I = 2429187.4 + 70.449d*E
             (JD2414600 - 34000) [00580]; since JD2426000 - see Table.
V0366 Cyg    Min II 10.2.
V0367 Cyg    VB A (A 0.1", 50deg; B 13.7m, 2.3", 255deg). Min II 7.16.
             Shape of the light curve and the radial velocity curve
             vary.
V0368 Cyg    According to [00204] EB type (12.8m - 13.8m pg)
             with the elements: Min I = 2425808.10 + 0.47586d*E
             (JD2425805 - 853).
V0369 Cyg    P var. Max = 2438199 + 104.46d*E (JD2426000 - 38200);
             since JD2438200 - see Table.
V0370 Cyg    Min II 11.9. P var. Min I = 2425096.429 + 0.77453979d*E
             (JD2414400 - 30000); since JD2430000 - see Table.
V0371 Cyg    Min II 12.5.
V0374 Cyg    d = 0.03P.
V0380 Cyg    Min II 5.76; Min II - Min I = 0.418P (1963).
             There are periodic terms in the elements:
             +0.8916d*sin(38.8deg + 0.0082deg*E) -
             0.0796d*sin(77.6deg + 0.0164deg*E) + 0.0088d*cos(26.4deg +
             0.0246deg*E); Min II = 2441262.266 + 12.425612d*E -
             0.8916d*sin(38.8deg + 0.0082deg*E) - 0.0796d*sin(77.6deg +
             0.164deg*E) - 0.0088d cos (26.4deg + 0.0246deg*E).
             Apsidal motion is possible with P = 1490 years.
V0382 Cyg    VB A (B 11.5m, 11", 332deg). Min II 9.12.
             Shape of the light curve and depth of Min II vary. P var.
             Min I = 2427992.458 + 1.885497d*E (JD2413480 - 29500)
             [01253]; since JD2428000 - see Table.
V0385 Cyg    Min II 12.4.
V0387 Cyg    Min II 11.6.
V0388 Cyg    Min II 9.15; d = 0.06P. P var. Min I = 2433584.540 +
             0.8590507d*E (JD2427600 - 37200);
             since JD2437200 - see Table.
V0389 Cyg    VB A (B 8.0m, 3.4", 305deg, 1980). SB (P = 3.313168d);
             Turns around the invisible third companion with
             P = 154.09d. According to [01256] the light varies with
             two alternate periods P1 and P2. The first oscillation
             (P1) with A = 0.19m satisfies the elements: Max =
             2423298.460 + 1.12912d*E, the second (P2) with A =
             0.05m - the elements: Max = 2429162.080 + 1.19328d*E.
             each of them continues for 1 - 3 weeks. At the transition
             from one oscillation to the other irregular light
             variations are sometimes observed or almost constant
             brightness. At the renewal of each oscillation its phase
             remains unchanged, experiencing no shift. According
             to [08909] in 1975 - 1977 periodicity was not observed.
V0393 Cyg    d = 0.02P.
V0401 Cyg    Min II 11.13. P var. Min I = 2432881.277 + 0.582717d*E
             (JD2428800 - 34000); since JD2434000 - see Table.
V0402 Cyg    VB A (B 20", 90deg).
V0407 Cyg    VB A (B 14.0m, 8", 190deg).
             Light variations of the Mira type
             variable are superimposed by the outburst of the probable
             nova which occured near JD2428400 (1936)
             with the consequent slow light decrease. Combined spectrum.
V0411 Cyg    P var. Max = 2421075 + 321d*E (JD2421000 - 31100)
             [01262]; since JD2431100 - see Table.
V0416 Cyg    Red.
V0425 Cyg    Description of the spectrum and its variations [02685, 03149].
V0427 Cyg    P var. Max = 2425471 + 143d*E (JD2425400 - 5950)
             [01155]; since JD2433850 - see Table.
V0429 Cyg    In the region of the open cluster NGC 6883.
V0430 Cyg    In the region of the open cluster NGC 6883.
             Max = 2425544 + 258d*E (JD2425500 - 27400) [01155].
V0432 Cyg    In the region of the open cluster Dolidze 3.
V0439 Cyg    In the region of the open cluster Berkeley 87 = OCL 161.
V0441 Cyg    Epoch of Min I is given.
V0442 Cyg    Min II 10.4:, d = 0.01P:. According to
             [08721] the period given in [00525] must be doubled.
V0443 Cyg    There is a periodic term in the elements:
             -0.016d*sin(0.00105*E).
V0444 Cyg    In the H II region S 109. Min II 8.06;
             D II  = 0.10P. P var. Min I  = 2430856.453 + 4.21238d*E
             (JD2415000 - 30000) [00007]; since JD2430000 - see Table.
V0445 Cyg    P var. Min = 2425527.391 + 1.947833d*E (JD2425500 -
             34700) [01155]; since JD2434700 - see Table.
V0447 Cyg    In the region of the open cluster NGC 6871.
V0448 Cyg    In the region of the open cluster NGC 6871. Min II 8.40.
V0450 Cyg    The light curve resembles that of DQ Her.
V0453 Cyg    In the region of the open cluster NGC 6871. Min II 8.68;
             d = 0.03P; Min II - Min I = 0.5077P. [07518]. According to
             [07518] there is apsidal motion with P = 71 years.
V0454 Cyg    Min II 12.3. In the region of the open cluster IC 4996.
V0455 Cyg    Min II 10.9. P var. Min I = 2431151.908 + 8.7689331d*E
             (JD2426800 - 33950) [01286]; since JD2436800 - see Table.
V0456 Cyg    Min II 11.4; Min II - Min I = 0.518P. P var?
V0457 Cyg    Min II 13.9.
V0458 Cyg    Min II 14.2.
V0461 Cyg    PB ~7000d? [08251].
V0462 Cyg    P var. Max = 2428540 + 376.0d*E (JD2416000 - 35200);
             since JD2435200 - see Table.
V0463 Cyg    Min II 10.65; Min II - Min I = 0.514P.
V0465 Cyg    There is a close companion of 17.5m.
V0466 Cyg    Min II 11.4.
V0469 Cyg    Min II 12.9; Min II - Min I = 0.57P.
V0470 Cyg    Min II 8.545.
V0471 Cyg    S 5.5/5.5.
V0473 Cyg    P var. Max = 2430615 + 218.5d*E (JD2418000 - 31000)
             [00346]; since JD2442300 - see Table.
V0474 Cyg    d = 0.014P.
V0477 Cyg    Min II 8.69; D II = 0.09P; d = 0.003P. P var. Min I =
             2429194.309 + 2.3470011d*E (JD2410000 - 29200)
             [00001]; Min I = 2437317.2695 + 2.3469943d*E
             (JD2429200 - 39700) [08919]; since JD2439700 - see Table.
             Apsidal motion with Pi = 349 years; E = 0.302 [06175].
             0.331P (1965 - 1970) <= Min II - Min I < = 0.460P (1904).
V0478 Cyg    VB A (B 12.8m, 4", 259deg. Min II 9.02; Min II - Min I =
             0.5072P.
V0482 Cyg    VB A (B 14.4m V, M4 III, 8", 225deg).
V0483 Cyg    Min II 11.9.
V0484 Cyg    Min II 13.6.
V0486 Cyg    Min II 14.3.
V0488 Cyg    Min II 13.0.
V0490 Cyg    Min II 13.5; Min II - Min I = 0.47P.
V0491 Cyg    Min II 14.7.
V0493 Cyg    Min II 12.9.
V0494 Cyg    Min II 13.6.
V0496 Cyg    Min II 12.5.
V0498 Cyg    Min II 10.27.
V0500 Cyg    VB B (A 11.5m; 18", 45deg). Min II 12.0.
V0501 Cyg    Min II 13.1; d = 0.02P.
V0502 Cyg    Min II 14.2.
V0505 Cyg    Min II 12.0.
V0509 Cyg    d = 0.05P.
V0512 Cyg    Min II 11.5. There is a periodic term in the elements:
             +0.065d*sin(0.2105263deg*(E + 538)).
V0513 Cyg    Min II 12.6.
V0519 Cyg    Min II 13.4.
V0520 Cyg    VB A (B 15", 135deg).
V0525 Cyg    d = 0.03P:.
V0526 Cyg    Min II 13.1. In the region of the open cluster TGC 7039.
V0532 Cyg    P var. Max = 2434618.158 + 3.283651d*E (JD2427900 -
             35000); Max = 2436817.694 + 3.282792d*E (JD2435000 -
             38700); since JD2438700 - see Table.
V0536 Cyg    d = 0.010P.
V0538 Cyg    B - V: +1.17, +1.50.
V0539 Cyg    P2 = 1500d.
V0541 Cyg    Min II 10.9; DII = 0.012P; Min II - Min I = 0.453P.
V0544 Cyg    P var?
V0546 Cyg    Min II 15.2:; Min II - Min I = 0.48P; d = 0.077P.
             In the dark nebula Barnard 144.
V0547 Cyg    B - V: +1.27, +1.73. In the dark nebula Barnard 144.
V0548 Cyg    Min II 8.62. P var. Min I = 2442279.3838 + 1.80524695d*E
             (JD2430800 - 42300) [08930]; since JD2442300 - see Table.
V0563 Cyg    P var. Max = 2427590 + 295.4d*E (JD2426000 - 30250);
             since JD2430250 - see Table.
V0567 Cyg    d = 0.036P.
V0581 Cyg    Red.
V0586 Cyg    In the region of the open cluster NGC 7039.
V0588 Cyg    VB A (B 18m, 15", 0deg). Very Red.
V0589 Cyg    VB.
V0606 Cyg    P var. Max = 2428376.7 + 50.245d*E (JD2427950 - 31330)
             [01262]; since JD2437100 - see Table.
V0612 Cyg    Cycles of 50 - 100d (JD2427950 - 31330) [01262];
             since JD2437100 - see Table.
V0614 Cyg    Min II 14.5.
V0618 Cyg    In the region of the open cluster TGC 7092.
V0622 Cyg    In the region of the open cluster NGC 7092.
V0628 Cyg    Min II 12.5.
V0635 Cyg    Min II 13.5.
V0643 Cyg    P var. Elements given in the
             Table are valid in the interval JD2427950 - 31330.
V0644 Cyg    VB A (B 15.6m, 6", 141deg; C 16.3m, 6", 141deg).
V0645 Cyg    Observed as the
             bright nebular condensation with ~2" diameter scattering
             light of an O8 star associated with it but invisible
             because of absorption. A part of strongly polarized
             bipolar nebula with diameter about 10". There are
             strong emission lines of H, Fe II, [O I], [S II], etc. In
             the spectrum [08942, 09129]. H2O maser source. Infrared
             source CRL 2789.
V0651 Cyg    Min II 14.7.
V0652 Cyg    Min II 12.1.
V0664 Cyg    d = 0.05P.
V0666 Cyg    P var. Max = 2427965 + 236d*E (JD2427950 - 31350)
             [01262]; since JD2433400 - see Table.
V0670 Cyg    sp component of a close binary.
V0680 Cyg    Min II 10.3.
V0685 Cyg    VB.
V0687 Cyg    Min II 10.4. P var?
V0688 Cyg    d = 0.029P.
V0690 Cyg    d = 0.021P.
V0691 Cyg    d <= 0.034P.
V0692 Cyg    Min II 14.9?
V0693 Cyg    Min II 14.4?
V0694 Cyg    d = 0.017P.
V0695 Cyg    31 Cyg. Probably enters a common system with V1488 Cyg
             (32 Cyg). VB A (B 13.0m, 36.8", 332deg; C 6.99m, 107.0",
             174deg; D 5.0m, 338", 323deg). d = 0.0151P.
             Interferometric binary eclipsing system (A = 0.08",
             E = 0.15 [01582]; 0.035", 141.8deg, 1980.4). The epoch of
             eclipse of the component of the spectral type B4 by the
             component of the type K4 is given in the Table. The
             amplitude strongly varies depending upon the wavelength:
             A(lambda 6560 A) = 0.03m, A(lambda 3530 A) = 1.80m [09131].
V0696 Cyg    Mean magnitude varies with P = 1600d.
V0700 Cyg    Min II 12.3. P var. Min I = 2432028.863 + 0.340047d*E
             (JD2431700 - 37500) [05352]; since JD2437500 - see Table.
V0704 Cyg    Min II 14.2.
V0706 Cyg    Min II 13.9.
V0713 Cyg    Min II 15.1.
V0720 Cyg    P var. Min I = 2427611 + 332d*E (JD2429450 - 32000)
             [00798]; since JD2432500 - see Table.
V0726 Cyg    Min II 12.8; d = 0.018P.
V0728 Cyg    P var. Min = 2425760.475 + 2.0601256d*E (JD2425500 - 35000)
             [00164]; since JD2439700 - see Table.
V0729 Cyg    VB A (B 13.5m, 1.5", 65deg). Min II 9.29. P var. Min I =
             2434264.638 + 6.597700d*E (JD2428700 - 37900)
             [00001]; since JD2439750 - see Table.
V0731 Cyg    VB.
V0735 Cyg    Depth of Min II 0.04m.
V0736 Cyg    Min II 16.5. Close to NQ Cyg.
V0737 Cyg    Star 23 - 50 [01321].
V0739 Cyg    Star 36 - 81 [01321].
V0741 Cyg    d = 0.03P.
V0742 Cyg    P var. Max = 2429409.448 + 0.93979d*E (JD2428420 -
             30700) [08977]; Max = 2431489.580 + 0.94010d*E
             (JD2430250 - 32350); Max = 2433282.014 + 0.93979d*E
             (JD2432350 - 33650); since JD2433650 - see Table.
             According to [08977] since JD2430700 the observations are
             better represented by the elements:
             Max = 2432943.701 + 0.93977897d*E - 1.067d*10**(-7)*E**2.
V0747 Cyg    The intervals between maxima of brightness
             are 2000 - 4000d. Not red.
V0751 Cyg    In the region of the nebula IC 5070. SB (P = 0.25d [09132]).
             Rapid small variations near maximum of brightness
             (<B - V> = +0.25) are superimposed sometimes by deep
             minima lasting for some hundreds days [02699]. Soft X-ray
             source [09133]. Spectrum description [02698, 09132].
V0752 Cyg    <B - V> = +0.77, <U - B> = -0.47.
V0753 Cyg    d = 0.12P. P = 0.952374d?
V0757 Cyg    Red.
V0758 Cyg    P = 400d?
V0759 Cyg    P var. Max = 2434513.427 + 0.36001476d*E
             (JD2414430 - 34570) [03506]; since JD2434500 - see Table.
             Blazhko effect.
V0779 Cyg    Type RR?
V0781 Cyg    P var?
V0783 Cyg    P var. Max = 2433261.029 + 0.62069487d*E
             (JD2424690 - 34000); since JD2438970 - see Table.
V0786 Cyg    Usually in minimum brightness, with rapid
             brightenings by 0.5m - 1.0m. In the interval JD2427692 -
             697 the brightness was 13.5m.
V0789 Cyg    P var? [Fe/H] = -0.91.
V0795 Cyg    sf component of a close pair.
V0796 Cyg    Min II 11.4.
V0797 Cyg    Min 15.4.
V0799 Cyg    P var.
V0801 Cyg    There is a square term in the elements:
             +1.93d*10**(-10)*E**2.
V0802 Cyg    P var. Max = 2432779.9342 + 0.59560377d*E
             (JD2425480 - 35170) [02775]; Max = 2439415.263 +
             0.5955638d*E (JD2435950 - 40000) [09266]. Max =
             2440036.409 + 0.595447d*E (JD2440000 - 41000); Max =
             2441517.498 + 0.595635d*E (JD2441000 - 42500);
             since JD2442500 - see Table. Shape of the light curve
             varies (0.13P <=  M - m <= 0.50P); period variations are
             accompanied sometimes by strong variations of amplitude
             (in the interval JD2440000 - 41000; 0.3m <= A <= 1.7m).
V0803 Cyg    Min II 14.5.
V0806 Cyg    Min II 15.0; DII = 0.061P.
V0807 Cyg    Min II 14.9.
V0808 Cyg    Brightness in maximum varies.
V0809 Cyg    Min II 13.6; DII = 0.069P.
V0810 Cyg    d = 0.050P. Depth of Min II 0.05m. P var?
V0817 Cyg    sp component of the pair.
V0818 Cyg    Shape of the light curve and period vary.
V0821 Cyg    Min II 15.6.
V0822 Cyg    Min II 13.0.
V0824 Cyg    Min II 14.3.
V0825 Cyg    Min II 16.9. Min II = 2433871.915 + 7.709015d*E.
V0826 Cyg    Min II 14.7.
V0828 Cyg    Min II 10.12.
V0832 Cyg    VB A (B 9.43m, 20", 352deg; C 11.62m, 27", 141deg; D 12.72m,
             38", 220deg). description of spectral variations [09135].
V0836 Cyg    Min II 8.77. P var. Min I = 2426547.5224 + 0.65341090d*E
             (JD2425500 - 42000) [03869]; since JD2441200 - see Table.
             Shape of the light curve varies.
V0840 Cyg    LS II 28.3deg [08090]. Cycles 250 - 300d.
V0841 Cyg    Min II 11.2.
V0842 Cyg    Min II 14.1.
V0844 Cyg    VB A (B 17.8m, 2.9", 50deg).
V0850 Cyg    Min II 11.8. P var. Min I = 2430587.263 + 4.5578d*E
             (JD2428750 - 30590) [04253]; since JD2434330 - see Table.
V0851 Cyg    d = 0.017P?
V0852 Cyg    Min II 14.9.
V0853 Cyg    Min II 14.2.
V0856 Cyg    Depth of Min II 0.05m.
V0857 Cyg    Depth of Min II 0.03m.
V0859 Cyg    Min II 12.1.
V0865 Cyg    Min II 14.6.
V0866 Cyg    Min II 13.9.
V0869 Cyg    Min II 14.8. Shape of the light curve varies.
V0870 Cyg    Min II 15.8.
V0871 Cyg    Min II 14.9.
V0873 Cyg    Min II 14.7. Min II - Min I = 0.48P.
V0874 Cyg    Min II 13.8.
V0877 Cyg    Min II 12.9.
V0880 Cyg    Min II 14.1; Min II - Min I = 0.506P; d = 0.02P.
V0881 Cyg    Delta(S) is small [09037].
V0882 Cyg    [Fe/H] = -1.42.
V0884 Cyg    np component of a pair. Min II 14.2.
V0885 Cyg    Min II 10.2.
V0886 Cyg    Min II 14.1; Min II - Min I = 0.515P.
V0887 Cyg    Depth of Min II 0.03m.
V0888 Cyg    Min II 15.9.
V0889 Cyg    Min II 10.4.
V0891 Cyg    Min II 9.4.
V0892 Cyg    Min II 15.5. nf component of a close pair.
V0900 Cyg    Min II 15.2.
V0902 Cyg    d = 0.02P. Depth of Min II 0.05m.
V0906 Cyg    Min II 15.7.
V0907 Cyg    Min II 14.9. According to [04427] Min I =
             2435066.257 + 0.54138554d*E.
V0908 Cyg    nf component of a close pair. Depth of Min II 0.04m.
V0909 Cyg    Min II 9.66.
V0910 Cyg    Min II 14.2; d = 0.02P.
V0911 Cyg    Min II 14.6. P var? Min I = 2432120.251 + 3.42262215d*E
             (JD2415500 - 37900) [04761]; since JD2437100 - see Table.
V0912 Cyg    Depth of Min II 0.05m.
V0913 Cyg    VB A (B 17m, 0deg).
V0920 Cyg    A var. Blazhko effect?
V0922 Cyg    d = 0.02P:.
V0924 Cyg    P var. Max = 2435706.776 + 5.5709816d*E (JD2432760 - 38000)
             [08053]; since JD2438000 - see Table.
V0925 Cyg    Min II 16.0.
V0927 Cyg    Epoch of Min brightness is given.
V0928 Cyg    Min II 15.4.
V0931 Cyg    Min II 14.5.
V0932 Cyg    Depth of Min II 0.04m.
V0934 Cyg    Min II 13.7.
V0936 Cyg    Depth of Min II 0.05m.
V0939 Cyg    Min II 12.5.
V0940 Cyg    Min II 15.1.
V0941 Cyg    Min II 13.2.
V0942 Cyg    VB A (B ~10deg, C ~110deg).
V0944 Cyg    np component of pair.
V0947 Cyg    Min II 15.0.
V0948 Cyg    Min II 15.2.
V0949 Cyg    Red.
V0955 Cyg    Min II 15.3. sp component of a close pair.
V0956 Cyg    Min II 15.1. sp component of a close pair.
V0957 Cyg    Min II 12.6.
V0958 Cyg    P = 199d?
V0959 Cyg    Min II 11.4; Min II - Min I = 0.52P; DII = 0.16P:.
             sp component of a close pair.
V0961 Cyg    Min II 12.4; Min II - Min I = 0.505P.
V0962 Cyg    d = 0.02P:.
V0964 Cyg    Min II 14.4.
V0965 Cyg    Min II 14.9. Type RRC? P = 0.32028628d?
V0970 Cyg    Min II 14.8.
V0974 Cyg    Min II 12.5; Min II - Min I = 0.462P.
             Min II = 2435373.398 + 3.204418d*E.
V0979 Cyg    Min II 14.7.
V0981 Cyg    Min II 15.0.
V0982 Cyg    Red.
V0997 Cyg    [Fe/H] = -0.77.
V1004 Cyg    Min II 13.0.
V1007 Cyg    Depth of Min II 0.04m.
V1008 Cyg    Min II 16.0.
V1010 Cyg    Depth of Min II 0.03m.
V1011 Cyg    Depth of Min II 0.04m.
V1012 Cyg    Min II 15.4.
V1016 Cyg    Before the outburst in 1964 the brightness
             changed between 15.0m and 17.5m pg [05701], the spectral
             type was late Me alpha [01222]. In the 1964 - 67 the
             brightness increased from 16.0m to 11.2m B. In 1967 - 69
             the brightness steadily increased to 10.05m B,
             being constant in V system (10.5m). In the infrared it
             changes in the limits 6.9 - 8.4 J, 4.7 - 5.8 K with the
             period 470d [07174, 09141]. High excitation emission
             spectrum with strong IR excess resembles that of
             symbiotic variables [09142]. X-ray and radio source.
V1018 Cyg    Min II 11.6.
V1021 Cyg    Min II 14.3.
V1023 Cyg    Min II 12.9; d = 0.03P:. DII = 0.14P.
             Min II - Min I = 0.495P.
V1024 Cyg    Depth of Min II 0.04m.
V1030 Cyg    Elements given in the
             Table are valid in the interval JD2426600 - 32300.
V1033 Cyg    P var.
V1034 Cyg    Min II 9.9.
V1035 Cyg    P var?
V1037 Cyg    Min II 14.8.
V1038 Cyg    VB B (9.4", 215deg, 1963). Min II 15.5.
V1039 Cyg    Min II 15.6.
V1042 Cyg    VB A (B 10m, 53", 110deg). In HII region S 109.
V1044 Cyg    Min II 16.5.
V1045 Cyg    Min II 16.0.
V1047 Cyg    d = 0.02P.
V1053 Cyg    d = 0.05P.
V1057 Cyg    In the dark nebula, in the region of the North America
             nebula (NGC 7000). In 1969 - 70 (JD2440400 - 830)
             the outburst from 16.5m to 10.3m occured. Brightness
             maximum was observed at JD2440830 (spectrum - B3).
             Before the outburst the light changed in the range
             15.5m - 16.5m, the spectral type was Ke with
             characteristic features of T Tau type stars [02698, 06415].
             After the outburst the brightness began to weaken
             monotonouosly and in 1982 reached 13.1m B (the spectral
             type about G2 - G5 Ib). Strong Halpha emission appeared
             in 1971. There are also small rapid light fluctuations.
             Description of light variations [06504, 07115,
             07754, 08996]. The star is associated with a luminous
             arc-shaped reflection nebula. This nebula with length
             of about 3' appeared in 1971 and its brightness is
             gradually decreasing simultaneously with the fading
             of the star.
V1061 Cyg    Min II 9.5.
V1063 Cyg    P var. Max = 2428260 + 339d*E (JD2428260 - 30700);
             since JD2433500 - see Table.
V1064 Cyg    Min II 15.3.
V1068 Cyg    Min II 11.2; d = 0.070P.
             A migrating wavelike distorsion with an amplitude ~0.1m V
             is being observed outside eclipses [08999].
V1073 Cyg    Min II 8.57.
V1074 Cyg    Min II 14.8.
V1083 Cyg    Min II 11.2.
V1085 Cyg    Observations given in [07010] contradict the elements given
             in [07193]: Min = 2437856.592 + 2.8089d*E.
V1096 Cyg    d = 0.03P.
V1102 Cyg    Radio-quiet N galaxy. Absorption spectrum without emission
             lines; z = 0.0272.
V1111 Cyg    Blazhko effect is possible.
V1122 Cyg    Blazhko effect is possible.
V1130 Cyg    Min II 12.9.
V1136 Cyg    Min II 13.2. Eccentric orbit (E = 0.3). Apsidal motion is
             possible [08051].
V1141 Cyg    Min II 11.8.
V1142 Cyg    Min II 13.4.
V1143 Cyg    Min II 6.06; Min II - Min I = 0.743P; d = 0.002P.
V1157 Cyg    Min II 13.6.
V1158 Cyg    d = 0.02P; Depth of Min II 0.04m.
V1161 Cyg    d = 0.01P.
V1162 Cyg    Only one Max was observed (see Table). Thereafter - either
             invisible, or fairly constant (17.6m - 17.8m). Bluish.
V1171 Cyg    VB A (B 11.0m, 0.34", 71.2deg; 1979.5). Min II 10.3.
V1175 Cyg    Min II 16.5. P var. Min I = 2434629.545 + 1.3330d*E
             (JD2426620 - 34630); since JD2434635 - see Table.
V1176 Cyg    VB. Variable is probably the northern red component.
V1187 Cyg    In the nebula IC 1318B. Min II 11.19. P = 3.7675d?
V1188 Cyg    Min II 14.3.
V1189 Cyg    Min II 13.7. P var. Min I = 2437906.516 + 1.041908d*E
             (JD2426620 - 31240); since JD2437906 - see Table.
V1191 Cyg    In the nebula IC 1318B. VB A (B 13m, 11", 299deg; C 13m,
             11", 284deg). Min II 11.11. Shape of the light curve varies.
V1193 Cyg    Min II 14.3.
V1196 Cyg    Depth of Min II 0.05m.
V1200 Cyg    Min II 16.1:.
V1210 Cyg    Red.
V1212 Cyg    Red.
V1218 Cyg    VB A (B 17m, sf).
V1225 Cyg    VB A (B 16m V, B - V = +1.3m, 1.2", 270deg; C 15.0m V,
             B - V = +0.5m, 2.4", 270deg); P var? Max = 2428250 +
             384.2d*E (JD2428200 - 38250) [03160]; since
             JD2438500 - see Table.
V1236 Cyg    Red.
V1255 Cyg    Brightness in Max varies in the range 15.2m - 16.0m with
             possible elements: Max = 2439382.281 + 0.28619537d*E.
V1256 Cyg    Min II 14.1.
V1273 Cyg    Min II 16.5.
V1275 Cyg    In the region of the open cluster NGC 6819.
V1281 Cyg    Min II 15.4.
V1285 Cyg    Red.
V1302 Cyg    Depth of Min II 0.05m.
V1305 Cyg    Min II 11.5m - 11.7m (var).
V1307 Cyg    Considerable dispersion of mean light curve points.
V1315 Cyg    Min II 15.3.
V1316 Cyg    (P) > 100d.
V1318 Cyg    LkH alpha 225. Associated with a cometary nebula.
V1321 Cyg    P = 0.7281802d?
V1322 Cyg    In the region of the open cluster NGC 6913.
V1326 Cyg    Min II 11.8; Min II - Min I = 0.53P.
V1327 Cyg    Very red.
V1329 Cyg    In 1891 - 1964 light variations in the range 14.2m - 15.5m
             with deep minima to 18m; the minima are satisfied by the
             elements given in the Table; D = 0.1p; spectral type M
             [07235]. In 1964 - the outburst up to 12.1m. Then gradual
             brightness decrease superimposed by periodical
             variations with an amplitude near 1m. Light minima
             as before are satisfied by the elements given in the
             Table but the character of eclipses changed (probably
             because of appearance of a dense envelope ejected
             by one of the components of the system). After the
             outburst high excitation emission spectrum with IR
             excess is observed similar to the spectrum of symbiotic
             variables.
V1331 Cyg    Associated with a cometary nebula.
V1334 Cyg    VB A (B 7.9m, B5 - B8, 0.13", 26.1deg, 1975).
V1336 Cyg    According to [07010], RR? P = 0.5d?
V1341 Cyg    Cyg X-2. SB1. Halo object (nu = -220 km/s). Strong
             reflection effect changes the spectral type of the F
             component. Spectral line profiles vary. The lines of
             He II, KCa II, C III,and N III are in emission. The
             system has low and high states. During the low state the
             mean light curve is a double wave with the range
             15.1m - 15.4m B. Epoch of Min I given in the Table
             corresponds to the F star in superior conjunction;
             Min II 15.4. The eclipse of the accretion disk at the
             phase 0.5P in partial. Rapid light variability by 0.1m
             in 10 minutes and by 0.5m in several hours is
             superimposed. In the high states lasting
             for ~10d the mean light increases by 0.5m. Radio
             source at 8085 MHz, source of soft and hard X-ray
             emission from 0.1 to 60 KeV.
V1345 Cyg    Min II 15.0:.
V1354 Cyg    Depth of Min II 0.04m.
V1356 Cyg    Min II 10.4.
V1357 Cyg    Cyg X-1. SB1. The epoch of the inferior conjunction of the
             optical component is given in the Table. Min II 8.88. The
             shape of the light curve varies; Min II sometimes are not
             observed. The periodicity in the light curve variations
             as well as in polarization changes is possible with
             P = 78.4d [09021, 09022]. Rapidly variable X-ray source in
             wide range up to 3 MeV characterized by the change of high
             and low states. Light and X-ray variation with P = 294d
             is also detected [09154, 09156]. Variable and flare radio
             source at 2695 and 8085 MHz.
V1372 Cyg    P2 = 360d?.
V1374 Cyg    Min II 17.7.
V1384 Cyg    In the region of the open cluster NGC 6913.
V1396 Cyg    VB AB (10.26m V, 12.3m V; A = 0.1127", P = 29.33 Y
             [09026]); mu = 0.67", P = 113deg; A-SB 2 (mAb - mAa = 0.6m,
             P = 3.275631d [09025]). Probably all the three components
             of the system are variables of the UV Cet type, and
             according to [05716] also of the BY Dra type. The range of
             combined brightness of the system is given in the Table.
             Really the flare of AB component was observed in the
             spectrograms [09025].
V1401 Cyg    Min II 13.6.
V1410 Cyg    P > 400d.
V1411 Cyg    P = 1.553478d?
V1412 Cyg    Min II 15.5.
V1414 Cyg    Northern component of a close pair; d = 0.04P.
V1416 Cyg    Min II 14.7.
V1417 Cyg    Min II 13.1.
V1421 Cyg    In the region of the planetary nebula NGC 6857 = K3 - 50.
V1425 Cyg    Depth of Min II 0.31m.
V1427 Cyg    In the region of the open cluster M39.
V1429 Cyg    Min II 15.3.
V1430 Cyg    Min II 15.0.
V1436 Cyg    Min II 15.9, D II = 0.08P; Min II - Min I = 0.48P.
V1437 Cyg    Min II 16.0.
V1440 Cyg    In the region of the open cluster NGC 6819.
V1465 Cyg    Resembles an eclipsing variable.
V1478 Cyg    VB A (B 17m:, 3", 80deg).
             Compact radio source. extended structure centered at the
             star is observed at 5 Ghz. Bq [] star with the excess of
             infrared radiation of dust at T = 300degK. Description of
             the spectrum [07080, 07081, 07523, 09159, 09160].
V1479 Cyg    In the region of the nebula IC 5070.
V1481 Cyg    Min II 12.5. In the region of the open cluster NGC 7128.
V1485 Cyg    Identical to VES 28, as it follows from latter star's
             coordinates and magnitudes in [7095], but the star is
             actually invisible in the chart in [7095], where a faint
             companion, to 0.4'N of the variable, is erroneously marked.
             Similarly, it is identical to +29deg 104, judging from the
             latter star's photometry and spectral type from [4732];
             however, the star is plotted slightly offset (by 0.8' to E)
             in the chart in [4732].
V1488 Cyg    32 Cyg. Probably enters a common system with V695 Cyg
             (31 Cyg). 0 < d < 0.011P. P var.
             Min I  = 2420670.0 + 1140.1d*E (JD2411400 - 29700).
             Since JD2429700 - see Table.
             The epoch of the eclipse of the B4 type
             Component by the K5 type component is given. There
             is also small physical light variability of the K
             component [08896, 09161]. Depth of eclipses depends of lambda:
             0.04M V, 0.13m B, 0.27m (lambda 4243A),0.90m (lambda 3552A).
V1489 Cyg    NML Cyg. 17.0m: - 18.0m V, B>21M; I - K = +8.17.
             Very large IR exess due to expanding gaseous-dust envelope.
             In the area 2.5"*3.5" around
             the star the system of about 60 discrete sources of
             OH emission is detected [07461]; source of OH, H2O,
             SiO maser emission. Light variations are periodical
             (see also [09163]). The object may be a protostar being
             observed at the end of condensation process. The late
             spectrum arises probably in the extending envelope
             [09165, 09166].
V1490 Cyg    In the region of the nebula IC 5070.
V1491 Cyg    In the region of the nebula IC 5070.
V1492 Cyg    In the region of the nebula IC 5070.
V1493 Cyg    In the region of the nebula IC 5070. V1707 Cyg 10.5"P.
V1494 Cyg    In the region of the nebula IC 5070.
V1495 Cyg    In the region of the nebula NGC 7000.
V1497 Cyg    In the region of the nebula NGC 7000.
V1498 Cyg    In the region of the nebula NGC 7000.
V1500 Cyg    In August 1975, before the very rapid increase
             of light, the brightness of the Nova gradually increased
             from 17.6m to 13.5m B (JD2442632 - 653.2). After Max
             almost monotonous decay of brightness is superimposed by
             light variations with the amplitude of 0.03m - 1.0m V;
             the period of these variations in the interval
             JD2442656 - 43100 changed in the range 0.1415d [09167,
             09168] - 0.137d [09169, 09170].  Since JD2443100 Min =
             2443696.4827 + 0.1396133d*E. Some investigators (see,
             for instance, [09173]) adopt double value of this peiod.
             A month after the light maximum of the Nova the
             radio emission was registered at 2695 and 8085 MHz [09171].
V1507 Cyg    The epoch of a broad Min I (superior conjunction of
             the B component) is given; Min II 7.01; D II = 0.20P,
             Min II - Min I  = 0.29P; e = 0.39. Unusual light curve
             [08213, 09049]. Shape of the light curve and depths of
             Min vary. Gaseous streams And expAnding envelope.
V1508 Cyg    Min II 13.3.
V1509 Cyg    VB A (B 11.7m, 55", 106deg).
V1511 Cyg    V - K = 13.6m.
V1513 Cyg    Gliese 781; mu alpha = -0.146S, mu delta = -1.00"; SB.
V1515 Cyg    In a dark nebula,  near the nebula NGC 6914. Connected
             with nebular appendage like a Comma. Light increase was
             observed from 1944 till 1958. Since 1958 the star is in
             Max. Slow light variations with A <= 1.6m. The absorption
             line Li I lambda 6707A is seen in the spectrum.
V1521 Cyg    Cyg X-3. Peculiar infrared X-ray source. V > 23m.
             Flare radio source. In the K band short and slow flares
             on the time scale about 2 minutes and 1-2 hours,
             irregular variations and longperiodic variability are
             observed [07752]. These variations are accompanied
             by periodical oscillations of infrared, X-ray and gamma
             radiation with the elements: Min = 2440949.8986 +
             0.1996830d*E + 1.25d*10**(-10)*E**2 [09187]. Usually the
             amplitude of these variations A(K) = 0.5m, but sometimes
             they disappear completely.
V1523 Cyg    Amplitude and mean brightness strongly vary.
V1531 Cyg    LkH alpha 142. VB A (B = V1532 Cyg, 2.5", 90deg). In the
             region of the nebula IC 5070. Combined brightness and
             spectrum are given.
V1532 Cyg    LkH alpha 143. VB B (A = V1531 Cyg; B 2.5", 90deg).
             In the region of the nebula IC 5070. Combined brightness
             and spectrum are given.
V1535 Cyg    In the region of the nebula IC 5070.
V1536 Cyg    In the region of the nebula NGC 7000.
V1538 Cyg    In the region of the nebula NGC 7000.
V1539 Cyg    In the region of the nebula NGC 7000.
V1540 Cyg    In the region of the nebula NGC 7000.
V1546 Cyg    In the region of the nebula NGC 7000.
V1548 Cyg    VB A (B 16.7m, 6.2", 131deg).
V1554 Cyg    VB A (B 14.7m, 3.5", 214deg).
V1577 Cyg    In the cluster and nebula IC 5146.
V1578 Cyg    In the cluster and nebula IC 5146. VB A (B 15m, 5", 45deg;
             C 17m, 5", 225deg). Associated with a reflecting nebula.
V1580 Cyg    There is a periodic term in the elements:
             -0.027d*sin(0.045deg) (JD - 2439000).
V1581 Cyg    G 208 - 44. VB A (B = G 208 - 45, 15.97m V, M6Ve; 7.9",
             106deg, 1954; 8.2", 96deg, 1974). mu = 0.71", P = 140deg.
             The flare was observed during spectroscopic observations
             [09175]. The companion may be also a UV Cet type variable.
             The range of combined brightness variation of the system
             is given.
V1584 Cyg    Epoch of min brightness is given.
V1597 Cyg    In the region of the nebula IC 5070.
V1598 Cyg    In the region of the nebula IC 5070.
V1600 Cyg    In the region of the nebula IC 5070.
V1608 Cyg    In the region of the nebula NGC 7000.
V1610 Cyg    Infrared source CRL 2688, the star of the spectral type
             F5Ia, associated with a bipolar reflection nebula
             (the so-called Egg nebula). The northern component of
             the nebula is 4" to the north from the source. Since 1920
             to 1958 the integrated light of this component increased
             from 15.2m to 13.4b B and after that does not vary [08735]. Light
             of the faint (16.2m B) southern component (5" to the
             south from the source) varies by 0.6m B [09176]. The
             radiation of the nebula is strongly polarized (46%,
             theta = 106deg in V system). There are C3 absorption
             features as well as Na, C2, and [S II] emission in the
             spectrum. Probably the object is a precursor of a
             planetary nebula [09178].
V1611 Cyg    In the region of the nebula NGC 7000.
V1624 Cyg    A var.
             In 1957 out of a B star turned into Be star. Probably must
             be referred also to GCAS type.
V1661 Cyg    VB A (B 11.14m, 20", 174deg).
V1668 Cyg    There are sinusoidal light variations with A(V) = 0.15m
             and elements Min = 2443767.475 + 0.4392d*E in the
             descending branch of the light curve after JD2443765
             [09179]. Infrared light curves (1.6 - 10 mkm) have a
             secondary maximum (JD2443815) due to the formation of
             the dust envelope. At 10 mkm this secondary maximum is
             brighter than the primary one [09069].
V1669 Cyg    d = 0.036P.
V1671 Cyg    Delta(U) = 0.06.
V1674 Cyg    VB (B 15m, 5").
             The range of combined brightness variation is given. It
             is not excluded that it is the component B that is
             variable. Slow variations of mean brightness in the range
             10.555m - 10.570m B are superimposed by sinusoidal
             periodikal ones with P1 = 1.3608d (A1 = 0.0037m)
             and P2 = 0.8055d (A2 = 0.0032m).
V1676 Cyg    In the open cluster NGC 6871.
             ADS 13374 A (B 12.0m, 6.5", 64deg; C 11.0m, 9.5", 28deg
             D 9.5m, B3V, 11.4", 301deg; E 11.42m, 28.1", 109deg;
             F 7.36m, B1IA, 35.9", 29deg); SB2 (P = 112.7d).
V1696 Cyg    SB1 (Porb = 4.3174d). Epoch of Min brightness is given.
             The eclipse of the accretion disc around the compact
             object formed in the outburst of a Supernova in a binary
             system about 5*10**6 years ago is possible [03619].
V1701 Cyg    In the region of the nebula IC 5070.
V1702 Cyg    In the region of the nebula IC 5070.
V1703 Cyg    In the region of the nebula IC 5070.
V1704 Cyg    In the region of the nebula IC 5070.
V1706 Cyg    In the region of the nebula IC 5070.
V1707 Cyg    In the region of the nebula IC 5070. V1493 Cyg 10.5"f.
V1711 Cyg    In the region of the nebula NGC 7000.
V1716 Cyg    In the region of the nebula NGC 7000.
V1719 Cyg    Shape of the light curve varies.
V1720 Cyg    Min II 7.79.
V1721 Cyg    P var.Min I = 2442605.497 + 2.724370d*E (JD2442311 - 928);
             since JD2442928 - see Table.
V1722 Cyg    Min II 14.6?
V1726 Cyg    Possible member of an anonimous open cluster.
V1727 Cyg    4U 2129 +47. Lx/Lopt ~10.
             Emissions in the spectrum: NeII lambda 4686A, CIII - NIII
             lambda lambda 4640 - 50A.
V1735 Cyg    In the complex of dark nebulae associated with the
             open cluster and the nebula IC 5146. Lights up a
             reflecting nebula. Became brighter by 5m at least
             from 1952 to 1965.
V1737 Cyg    B - V = +3.7.
V1738 Cyg    B - V = +5.5:.
V1739 Cyg    B - V = +4.5:.
V1744 Cyg    Epoch of Max in U system is given.
V1746 Cyg    Sometimes P = 0.21d is observed.
V1747 Cyg    P > 100d. B - V = +4.0.
V1748 Cyg    In the nebula IC 1318a.
V1751 Cyg    In the nebula IC 1318c.
V1761 Cyg    Close companion? Elements are not certain.
V2105 Cyg    Variability type and spectral type (F8Iab:) do not agree.
V2121 Cyg    Strong Blazhko effect.
V2150 Cyg    Type RR: is also possible.
V2174 Cyg    SB, Porb = 225.162d.
V2175 Cyg    X-ray source.
V2312 Cyg    Erroneously called HD 192776 in [190].
V2324 Cyg    Possible brightening trend over 6 years, maybe due to dissipating
             dust envelope, plus quicker variations.
alf   Cyg    VB A (B 11.4m, 75.3", 106deg).
tau   Cyg    VB A (B 6.44m, G1V, A = 0.88", P = 49.80yr; C 12.20m,
             29", 230deg). 0.083d <= P <= 0.125d.
             The range of total light variation is given.
ups   Cyg    VB A (B 10.2m, 15.2", 220deg; C 10.2m, 21.5", 180deg).
khi   Cyg    VB A (B 10.8m, 158", 254deg). S 6 + %1e (Tc). SiO
             maser. P var.Max = 2393559 + 405.88d*E (JD2337150 - 94000);
             since JD2394000 - see Table.
P     Cyg    The appearance of the star was firstly noted in
             1600, when its brightness was 3m. Since the XVIII
             century the light of the star varies in the range
             4.6m - 5.6m vis. Radio source at the millimetre and
             centimetre wavelengths.
Q     Cyg    In minimum brightness varies periodically with the
             amplitude 0.5m: Max = 2440495 + 54.99d*E; P = 64.81d is
             also possible. Mean level of brightness varies in the
             range 15.2m - 15.9m B.
S     Del    VB A (B 56", 342deg). Double maxima are sometimes observed.
U     Del    Mean brightness var, P = 1100d. According to [08993], the
             period value 160d - 180d is more likely than 110d.
W     Del    d = 0.017P. Min II 9.79. P var. Since JD2433000 - see
             Table. The light curve shape var.
RZ    Del    VB (A var; B var, 17", 137deg) [03771].
TT    Del    P var. Since JD2435000 - see Table.
TW    Del    Delta(m) var (0.5m + 3.4m).
             The light curve resembles that of RV Tau, with Min I and
             Min II; the epoch of Min I is given.
             Min I = 2432171.1 + 118.4d*E (1947 - 1952);
             Min I = 2435386.8 + 115.9d*E (1955 - 1963); during
             1964 - 1970 - see Table.
TX    Del    P var. P = 6.166585d (JD2428000 - 36600); since
             JD2436600 - see Table.
TY    Del    Min II 9.8. P var.Min = 2428020.399 + 1.191121d*E
             (JD2428000 - 38000) [00279]; since JD2438000 - see Table.
TZ    Del    Epoch of Min is given.
VV    Del    Depth of Min II 0.05m.
YY    Del    Min II of the depth ~0.05m is possible. P var.
             Min = 2425795.488 + 0.7930856d*E (JD2425000 - 34000)
             [01329]; since JD2434000 - see Table.
AL    Del    Min II 12.4.
BG    Del    Min II 13.8.
BK    Del    P var?
BR    Del    Emission.
BX    Del    Delta(S) = 0.
BY    Del    Min II 11.8.
CE    Del    [Fe/H] = -0.68.
CF    Del    The light curve shape var?
CH    Del    [Fe/H] = -1.23. According to [09037], P = 0.315D.
CN    Del    Min II 14.6.
CR    Del    Min II 13.7.
CS    Del    [Fe/H] = -0.92.
CU    Del    Abrupt phase chande was noted.
CW    Del    P var.P = 0.58209d (JD ~2427100), P = 0.58211D
             (JD ~2428800); During JD2429800 - 30600 - see Table.
DG    Del    The elements should be checked.
DK    Del    Min II 14.2.
DM    Del    Min II 8.80.
DT    Del    Epoch od Min is given. The elements are valid during
             JD2425480 - 6260.
DX    Del    [Fe/H] = -0.11.
EG    Del    P var. Max = 2425535.42 + 0.3248545d*E (JD2425478 - 30619)
             [00911]; abrupt change near JD2432578, since then see Table.
EI    Del    The mean brightness var, P ~600d.
EK    Del    B - V: +0.29, +0.53.
ES    Del    Epoch of Max from [03715], [07527] contradict the given
             elements.
ET    Del    Min II 12.7.
EW    Del    Min II 15.5.
EX    Del    Min II 13.3.
FI    Del    Min II 14.5.
FK    Del    Min II 14.5.
FM    Del    Delta(S) = 0.
FP    Del    [Fe/H] = -1.44.
FR    Del    Min II 15.3.
FT    Del    Blazhko effect?
GG    Del    Min II 12.6. P var?
GN    Del    P var? Delta(m) var?
GY    Del    VB B (A = BD +15deg 4134A, SP A - F).
HR    Del    Porb = 0.170920d. The brightness began to increase on
             JD ~2439653. Waves with maxima on JD2439752 (4.55m),
             2439799 (4.64m), followed by a sharp main Max, flat max on
             JD2439981 (4.09m) and final decline. Radio source.
HU    Del    mu = 0.685", theta = 79deg. Astrometric binary
             (semiamplitude of deviations 0.118", Porb = 1.52yr).
II    Del    [Fe/H] = -1.30.
IO    Del    A single outburst  was observed (JD2439378 - 388).
IV    Del    D ~0.1d.
LS    Del    Min II 8.76.
del   Del    (k - b)2 = 0.19. SB2 (Porb = 40.58d; e = 0.7).
             Spectra of both SB components show Am features; Fe, Ca,
             Sc deficiency, Sr, Y, Zr, Ba, Ce, La, Eu excess.
             Both components are DSCT variables; the period of the
             main component pulsation is 0.158d, that of the
             secondary is 0.134d [07528]. Any of the oscillations may
             occasionally dominante in the combined brightness:
             according to [07529], Max = 2439338.4444 + 0.135547d*E;
             according to [07530], P = 0.154991d.
R     Dor    VB A (B 11.9m, 34", 10deg; C 11.0m, 35", 130deg, 1933).
             H2O, SiO, HC3N emission.
S     Dor    VB A (B 12.1m, 13"). The member of the large magellanic
             cloud. In the cluster NGC 1910 and a diffuse nebula.
             One of the absolutely brightest stars. Deep Min: 1891,
             1900, 1930, 1940, 1955, 1964.
T     Dor    VB A (B 12.0m vis, 5", 13deg.)
V     Dor    At the edge of the Large Magellanic Cloud.
RR    Dor    In the region of the Large Magellanic Cloud. Min II 14.5.
RW    Dor    In the region of the Large Magellanic Cloud.Cloud
             non-member. P var [09036]. Min II 11.2.
RX    Dor    In the region of the Large Magellanic Cloud. Cloud
             non-member?
SW    Dor    In the region of the Large Magellanic Cloud.
             Cloud non-member. P var [09036].
SX    Dor    In the region of the Large Magellanic Cloud,
             Cloud non-member. Delta(m) var.
SY    Dor    In the region of the Large Magellanic Cloud.
             According to [09036], variability is doubtful.
SZ    Dor    In the region of the Large Magellanic Cloud, cloud
             non-member.
TY    Dor    In the region of the Large Magellanic Cloud, cloud
             non-member.
UU    Dor    In the region of the Large Magellanic Cloud,cloud
             non-member.
UV    Dor    In the region of the Large Magellanic Cloud,cloud
             non-member.
UX    Dor    In the region of the Large Magellanic Cloud, cloud
             non-member.
XX    Dor    In the region of the Large Magellanic Cloud, cloud
             non-member. [Fe/H] ~-1.3.
ZZ    Dor    In the region of the Large Magellanic Cloud, cloud
             non-member.
AA    Dor    d = 0.02P. Min II 11.21.
alf   Dor    VB A (B 4.3m, A = 0.2125", P = 13.00yr.)
             The range of combined brightness variations is given.
bet   Dor    P var. Current elements are given.
T     Dra    ADS 10937 A (B = UY Dra, optical, 16", 222deg).
U     Dra    P var. Mean elements are given.
W     Dra    P var. Max = 2416748 + 257.11d*E (JD2416750 - 21390);
             Max = 2430826 + 262.11d*E (JD2421390 - 30820);
             Max = 2439962 + 268.87d*E (JD2430820 - 40490);
             since JD2440490 - see Table.
Y     Dra    According to visual observations, 7.8m - 15.0m.
Z     Dra    Min II 11.0. P var. Min = 2430973.314 + 1.3574176d*E
             (JD2428460 - 33300); Min = 2433268.708 + 1.357440d*E
             (JD2433300 - 43500); since JD2443500 - see Table.
RR    Dra    d = 0.015P. Min II 10.1. P var. Before JD2439000
             Min I = 2433390.458 + 2.83123d*E [01001];
             since JD2440000 - see Table.
RS    Dra    During JD2436012 - 37584 P = 145.3d.
             Delta(m) and the light curve share vary strongly.
RW    Dra    P var. Mean elements are given.
             Composite Blazhko effect;
             Pi = 93.95P = 41.61d; Pi1 = 280P; Pi2 = 6140P; Pi3 =
             3400P [01585]. 0.11P <= M - m <= 0.32P. Delta(S) = 3.
RX    Dra    Min II 10.3, d II = 0.009P.
RZ    Dra    Min II 10.38. P var. Min = 2429448.787 + 0.55087668d*E
             (1907 - 1968) [03822]; since 1968 - see Table.
SU    Dra    P var. Before 1955 Max hel = 2420605.762 +
             0.66041890D; since 1955 - see Table. [Fe/H] = -1.39.
SW    Dra    Delta(S) = 3.5.
SX    Dra    d = 0.035P. Min II 10.0. P var. Min I = 2432273.276 +
             5.1692d*E (JD2432000 - 38000); since JD2442000 - see Table.
TT    Dra    P2 = 198d.
TW    Dra    ADS 9706 A (B 9.5m vis, 23deg, 3.6"). d = 0.02P;
             Min II 8.1. P var. Min I = 2433888.452 + 2.806870d*E
             (JD2433000 - 40000) [03825]; since JD2440000 - mean
             elements in the Table.
TX    Dra    Mean magnitude var, P2 = 654d.
UU    Dra    Mean magnitude var, P2 = 960d.
UX    Dra    According to [09086], the light curve may correspond
             to the type E; SB, P ~340d.
UZ    Dra    d = 0.01P; Min II 10.6. Possibly P = 1.65d [03827].
VW    Dra    According to photoelectric observations, 6.28m - 6.32m V.
WW    Dra    Nonlinear term: -4.98d*10**(-9)*E2.
             ADS 10152A (B 9.67m, 8.2", 5deg). Depth of Min II 0.08m.
WZ    Dra    Delta(m) var strongly.
XY    Dra    Min II 13.7.
XZ    Dra    P var. Before JD2438000 Max = 2427985.648 + 0.4764944d*E
             [00188]. Epochs after JD2438000 are represented dy the
             elements in the Table only on average. Blazhko effect;
             according to [01474], Pi = 78d. [Fe/H] = -0.57.
ZZ    Dra    P var. Max = 2434509 + 274.5d*E (JD2416350 - 34600); since
             JD2437100 - see Table.
AE    Dra    Delta(S) = (4).
AF    Dra    VR var; SB?
AG    Dra    A soft X-ray source. Elements in the Table represent
             maxima in U band in 1974 - 1979 [09113].
AI    Dra    Min II 7.16, D II = 0.17P.
AP    Dra    Twice shorter period is possible.
AQ    Dra    Hbeta spectral line is probably filled in by emission.
AR    Dra    Min II 11.63.
AS    Dra    mu = 0.486", P = 289deg. SB. Delta(m) var.
             Large spatial velocity. The brightness
             varies with the phase of the orbital motion. Phases
             of Max and Min vary from cycle to cycle. The Table
             gives Porb [03075] and the epoch of the conjunction
             (G4 - star is behind).
AW    Dra    P var. since JD2430500 - see Table.
AX    Dra    Min II 11.0.
BE    Dra    Min II 11.5. The spectral type is late B.
BH    Dra    ADS 12019A (B Am, 9.25m, 10.8", 58deg). Min II 8.58.
BK    Dra    P var.Max = 2415150.817 + 0.592019d*E (JD2414900 - 16150)
             [00001]; since JD2416940 - see Table.
             Delta(S) = 8 in Max light.
BP    Dra    Min II 14.7.
BS    Dra    Min II 9.84.
BV    Dra    ADS 9537 A (B = BW Dra, 16.3", 358deg, 1980; C 12.69m).
             Min II 8.40.
BW    Dra    ADS 9537 B (A = BV Dra; C 12.69m). Min II 9.02.
BY    Dra    SB2 (Porb = 5.9750998d, e = 0.36). mu = 0.365", P = 150deg.
             Quasiperiodic variability :
             DM var, P var, (differential rotation), phase jumps.
             Flares up to Delta(U) = 1.07m.
CM    Dra    VB A (B SP = DC, 15.7m pg, 25.7", 22deg, common mu).
             mu = 1.619", p = 317deg, pi = 0.068", V nu = -118.6km/s.
             Min II 13.63. BY type variability: Delta(M) ~<= 0.05mV,
             P ~Porb. Flares: Delta(m) ~0.05.
CR    Dra    mu = 0.50", p = 168deg, pi = 0.048".
CX    Dra    SB, Porb = 6.69612d (with this period Delta(V) = 0.04m).
             Long-term cyclic variations: P ~2400d, Delta(V) ~0.2m.
             Flares ~0.1m. An X-ray source; the reflection effect is
             observed.
DE    Dra    d = 0.017P.
DG    Dra    Depths respective to Max I (” = 0.25); Min II 0.17m;
             Max II 0.01m.
DK    Dra    Porb = 64.44d.
             Epoch of Min is given. Both components show H and K CaII
             in emission.
DL    Dra    VB A (B 9.2m, 3.9", 318deg, 1982). P1 = 0.0825d, A1 =
             0.028m; P2 = 0.0837d, A2 = 0.026m.
DN    Dra    P = 109S. mu = 0.32", P = 153deg.
kap   Dra    IR excess.
phi   Dra    ADS 11311 (Delta(m) = 1.7m, 0.3", 288deg, 1967). A:SB, P =
             26.768d. The epoch of Max U light is given.
S     Equ    Min II 8.11. P var. Before JD2427000 Min =
             2423746.490 + 3.4360050d*E [01140]; Min =
             2437968.345 + 3.436072d*E (JD2427000 - 41000)
             [03432]; since JD2441000 - see Table.
             Gaseous streams; in Min light Halpha is in emission.
W     Equ    Min II 12.4. P var.
Z     Equ    A nearby star: 12.1m.
RT    Equ    P var strongly.
RW    Equ    Strong Blazhko effect.
RZ    Equ    Min II 12.2:.
SU    Equ    Min II 16.4.
SV    Equ    Depth of Min II 0.16m.
SW    Equ    Min II 15.6.
NU    Equ    ADS 14702A (B 11.6m, 2", 268deg; C 12.6m, 48", optical).
             The Table gives the pEriod of oscillations. Data on the
             periodicity of the rotational variability of light,
             spectrum and magnetic field are contradictory
             (17.492d, 314d, 1785.7d, 72yr).
V     Eri    Mean magnitude var, P2 = 1209d.
W     Eri    SiO, OH, H2O maser.
Z     Eri    P2 = 746.4d.
RU    Eri    Min II 9.62.
RX    Eri    [Fe/H] = -1.32.
RY    Eri    d = 0.025P.
RZ    Eri    d = 0.018P. The depth of Min II 0.04m pg.
SV    Eri    [Fe/H] = -1.83. P var. P = 0.71365272d (JD2414000 - 21000);
             P = 0.71370172d (JD2421000 - 26000) [00862];
             Max = 2426590.319 + 0.7137406d*E (JD2426000 -
             34000) [09195]; since JD2434000 - see Table.
TT    Eri    (B - V)Max = +0.255m.
TV    Eri    (B - V)Max = +0.53m.
TZ    Eri    d = 0.015P. P var. Min = 2426066.198 + 2.606097d*E
             (JD2426000 - 33500) [01490]; since JD2438200 - see Table.
UX    Eri    Min II 11.01. P var? Before JD2438500 Min I =
             2434368.570 + 0.4452820d [02494]; since JD2438500 - see
             Table.
UY    Eri    The shape of the light curve var. [A/H] = -1.6.
VW    Eri    Alternating P1 = 83.4d, P2 = 93.3d. Halo population.
WW    Eri    Min II 11.2.
WX    Eri    The depth of Min II 0.22m. The primary component var,
             DSCT:,  P1 = 0.16454d, P2 = 0.13721d.
YY    Eri    Min II 8.72. P var. Min I = 2433617.5198 + 0.321496212d*E
             (JD2433000 - 41500) [03850]; since 2441500 - see Table.
             X-ray source.
ZZ    Eri    Min II 14.4.
AN    Eri    Min II 14.9.
AO    Eri    d = 0.04P.
AS    Eri    Min II 8.42. X-ray source.
BB    Eri    (k - b)2 = 0.13.
BC    Eri    Min II 11.26:.
BK    Eri    Delta(S) = 8. P var.
BL    Eri    The elements should be checked.
BM    Eri    P > 20000d; D = 321d; d = 270d.
             Only one Min was observed. Outside Min, according to
             [05828], Delta(V) = 0.2m, Max = 2440643.0 + 30d*E.
BQ    Eri    Min II 10.9.
BV    Eri    Min II 8.42. dII = 0.06P.
BW    Eri    Min II 9.72.
BY    Eri    (k - b)2 = 0.06.
BZ    Eri    Min II 9.21.
CC    Eri    SB. mu = 0.310", P = 169deg, Pi = 0.083".
             Photometric P is close to Porb. X-ray source.
CI    Eri    VB (9.9m, 11.2m, 2", 106deg).
CO    Eri    Min II 9.1.
CS    Eri    (k - b)2 = 0.03.
CT    Eri    Min II 10.27.
CW    Eri    Min II 8.86, DII = 0.10P.
DL    Eri    P0 - see Table; P1 = 0.118795d [09206]; P2 = 0.0968d [09207].
DM    Eri    ADS 3380 (5.1m, 5.4m, 0.3", 161deg).
             Duplicity was observed only in 1877 and 1923.
DO    Eri    Epoch of Min is given. Oscillations with P ~6.14 Min, 7
             different frequencies have been found. Beat phenomenon,
             PB = 12.25d +-0.47d. Max of the oscillation amplitude
             almost coincides with Max of the magnetic field, the
             amplitude varies with Prot. Combined amplitude of
             oscillations 0.062m B.
DS    Eri    Min II 10.3. P var. Min = 2423147.25 + 0.827737d*E
             (JD2414869 - 23150); during JD2423150 - 31320 - see Table.
DW    Eri    ADS 3409 B (A 6.72m, G8III; B 9", 317deg).
DY    Eri    ADS 3093 C (A 4.43m V, K1V; B 9.51m V, DA, 82",
             105deg; BC A = 7", Porb = 252.1yr). mu = 4.05", P = 212deg.
             X-ray source.
DZ    Eri    Epoch is given for Max (y), Min (He I).
             P = 3.67d is possible.
EF    Eri    2A0311 - 227. VB A (B 15.8m, 18", 260deg). mu alpha =
             +0.147", mu delta = -0.070".
             Epoch of narrow Min in IR light is given. The complex
             phenomenon of eclipses is described in [04041].
             Oscillations with P ~20.2 and 13.7 Min. [09211]. Flickering.
EG    Eri    Epoch of Min in Y light is given.
EH    Eri    ADS 3305 A (B 10.8m, 1.45", 60deg, 1917).
HV    Eri    Type RRC: is also possible.
gam   Eri    ADS 2904 A (B 12.4m, 53", 242deg).
lam   Eri    Shell features are sometimes present in the spectrum.
nu    Eri    SB? P2 = 0.1735079d. Beat effect.
omi 1 Eri
             P0 - see Table. P1 = 0.1291d.
tau 4 Eri
             ADS 2472 A (B 9.9m, 6", 288deg; C 11m, 40", 99deg).
tau 9 Eri
             SB1 (Porb = 5.954d). P = 1.2135d is not excluded.
S     For    VB (9.2m, 9.3m, 0.28", 358deg, 1964).
             Found unusually bright only on one night
             by three experienced observers in europe; harvard
             photographs of the same night show it in normal brightness.
V     For    (B - V)Max = +0.26.
W     For    Min II is observed.
RX    For    (k - b)2 = 0.06.
RY    For    (B - V)Max = +0.535.
SS    For    (k - b)2 = 0.09.
SW    For    Delta(S) > 10:.
SY    For    SB2 [M + pec(eq)].
TZ    For    SB2. Possible P values:
             37.805d; 44.18d; 50.46d; 75.61d. DI = 1d.
R     Gem    VB A (B 11.4m pg, 173", 200deg, 1910). S 3.5/6e- S 6.5/6-.
S     Gem    VB A (B 11.1m, 70", 122deg).
T     Gem    S 3/4e.
U     Gem    Min = 2437638.82685 + 0.17690602d*E + 5.4d*10**(-12)*E**2
             [09215]. Depth of Min 0.5m - 1.0m.
             Spectrum description [09216].
V     Gem    P var. Max = 2407750 + 276.2d*E (JD2407700 - 15500);
             Max = 2415729 + 278.3d*E (JD2415600 - 21600); Max =
             2421839 + 269.8d*E (JD2421700 - 26500) [00458]; Max =
             2432580 + 281.3d*E (JD2427500 - 32600); Max =
             2434739 + 269.8d*E (JD2432600 - 35800);
             since JD2435800 - see Table.
W     Gem    P var. Max = 2429815.990 + 7.914553d*E (JD2413200 -
             31700); since JD2431700 - see Table. [A/H] = 0.2.
             There is possibly faint blue companion.
RR    Gem    P var. Max = 2415219.734 + 0.39729235d*E
             (JD2412000 - 18000); Max = 2418278.900 + 0.39727274d*E
             (JD2418000 - 21000); Max = 2422865.229 +
             0.39724027d*E (JD2421000 - 25000) [09217]; Max =
             2427150.267 + 0.3972596d*E (JD2426200 - 27850);
             Max = 2434806.289 + 0.3973103d*E (JD2428200 - 34900)
             [02392]; since JD2436000 - see Table. Blazhko effect,
             PB = 48d [03618], PB = 37d [09221]. Delta(S) = 3.
RW    Gem    VB A (B 11.04m, 20", 105deg; C 11.84m, 100", 120deg).
             Min II 9.74; d = 0.02P.
RX    Gem    VB A (B 12.65m, 45", 215deg). Min II 9.28; d = 0.004P.
             P var. Min I = 2417970.0 + 12.20868d*E (JD2415000 - 27500) [07534];
             since JD2427600 - see Table.
             There is a square term in the elements given in the Table:
             +2.25d*10**(-7)*E**2. Luminous gaseous ring surrounds the
             primary component of the system [07535].
RY    Gem    VB A (B 12.30m, 45", 240deg). Min II 8.75; d = 0.023P.
             P var. Min I = 2418015.333 + 9.300876d*E
             (JD2418000 - 33000) [08653]; since JD2433000 - see Table.
             Component of A type is surrounded by a luminous gaseous
             ring.
RZ    Gem    VB. P var. Max = 2429632.453 + 5.529716d*E
             (JD2415000 - 32400); since JD2432400 - see Table.
SS    Gem    9.9m <= Min II <= 10.7m.
SU    Gem    P var. Min I = 2429204 + 50.12d*E (JD2429200 - 355)
             [00310]; Min I = 2437772.5 + 50.39d*E (JD2437739 -
             39850); Min I = 2439856.6 + 50.10d*E (JD2439850 -
             40680); since JD2440680 - see Table.
             Mean brightness varies with the elements:
             Min = 2437953 + 680d*E; M - m = 264d.
             Amplitude of shortperiodical variations is 0.3m - 0.9m.
SW    Gem    Min brightness epoch is given.
SX    Gem    Min II 11.3; d = 0.05P:.
TX    Gem    Depth of Min II 0.04m; d = 0.017P:.
UV    Gem    VB A (B 19.5m, 7", 285deg).
WW    Gem    Min II 10.3.
WY    Gem    May be an eclipsing system similar to VV Cep. Atmospheric
             eclipse began probably in 1960 - 61, the mean phase of it
             being in 1968 [05730]. Variable magnetic field [01591, 04498].
             Intrinsic variability of blue component is also possible
             [07536].
YY    Gem    VB C (A 1.99m, B 2.85m, a = 6.06", P = 306.3 y; C 73",
             165deg, 1925); mu alpha = -0.0154s, mu delta = -0.108".
             Min II 9.59; Min II - Min I = 0.50P; D = 0.000P. X-ray
             source. P const [08655]. Both components are probably
             UV Cet type variables. Flare amplitude in the integrated
             light of the system reaches 0.3m V, or 1.8m U [09227].
AA    Gem    [A/H] = 0.0.
AC    Gem    Min II 11.3. P var. Min I = 2433649.30 + 1.661795d*E
             (JD2415000 - 36000) [01530]; since JD2430100 - see Table.
AF    Gem    VB A (B 14.8m, 2", 0deg). Min II 10.67.
             There is a square term in the elements given in the Table:
             -1.71d*10**(-10)*E**2.
AH    Gem    Min II 14.8:.
AI    Gem    Min II 14.0.
AL    Gem    Min II 9.85.
AN    Gem    Min II 13.3:; d = 0.037P.
AU    Gem    OH emission.
AV    Gem    Min II 12.8:.
AY    Gem    Min II 10.9.
AZ    Gem    Min II 12.4.
BB    Gem    VB A (B 12m, 25", 270deg).
BP    Gem    P var. Max = 2434120 + 243.9d*E (JD2418700 - 36600);
             since JD2436600 - see Table.
BT    Gem    Min II 14.0:.
CI    Gem    UG?
CM    Gem    Min II 15.0.
DL    Gem    VB A (B 13.1m, 18", 180deg).
DN    Gem    VB A (B 13.5m, 12", 16deg; C 12.0m, 80", 99deg).
DP    Gem    Min II 14.0. RRC? P = 0.2792d?
DX    Gem    P var. Max = 2433182.876 + 3.136226d*E (JD2425000 -
             34000); Max = 2435554.199 + 3.136955d*E
             (JD2434000 - 36500) [08300]; since JD2436500 - see Table.
EF    Gem    P var. Min = 2428108.49 + 6.10222d*E (JD2428500 -
             42800) [00407]; since JD2442800 - see Table.
EL    Gem    Min II 13.6.
EN    Gem    Min II 13.8.
EW    Gem    P var. Max = 2428495.686 + 0.523750d*E (JD2428100 - 30780);
             since JD2430780 - see Table.
EY    Gem    Min II 13.0.
FT    Gem    Min II 14.1.
GP    Gem    Min II 13.5.
GR    Gem    15.6 <= Min II <= 15.9.
GW    Gem    Min II 10.68.
GX    Gem    Min II 11.3.
GZ    Gem    P = 1.225290d?
HH    Gem    Min II 13.8.
HR    Gem    Min II 11.7.
HY    Gem    Min II 17.5.
II    Gem    P = 223d?
IP    Gem    Min II 14.5.
IR    Gem    In supermaxima there are superhumps with P = 102 Min
             [09232].
IZ    Gem    D >= 0.24d.
KN    Gem    The minor planet (123) Brunhild.
KQ    Gem    Min II 14.6.
KU    Gem    d = 0.05P.
KV    Gem    Epoch of Min of brightness is given. EW
             type is possible according to the spectrum [09037].
KZ    Gem    The cycle may be 129d.
LM    Gem    d = 0.02P.
LX    Gem    Red.
MO    Gem    Red.
MP    Gem    VB.
MU    Gem    Min II 14.9.
MZ    Gem    Min II 16.7.
NQ    Gem    In the spectrum of the carbon
             star the hydrogen emission lines and ultraviolet
             continuous emission appeared in February 1970 [06348].
NY    Gem    HD 47396 (Pec) = S 5438 = CSV 798 = CSV 6468.
             In the chart in [00156] the position of the variable is
             wrong.
OS    Gem    Oscillations with
             the period P1 given in the Table are superimposed
             by oscillations with the period P0 = 0.070d and smaller
             amplitude. P1/P0 = 0.78.
V0345 Gem    The variability may be due to the fainter (B) component.
zet   Gem    VB A (B 11.46m, 87", 84deg; C 7.56m, 97", 350deg). P var.
             Max = 2410640.42 + 10.15477d*E (JD2394600 - 2407150);
             Max = 2422366.187 + 10.15288d*E (JD2407150 - 22300);
             Max = 2426802.918 + 10.15172d*E (JD2422300 - 34500)
             [02392]; since JD2434500 - see Table.
             All the observations are satisfied also by the
             elements: Max = 2443785.444 + 10.150135d*E -
             5.24d*10**(-7)*E**2 [09029].
             May by a DCEPS type variable.
eta   Gem    VB A (B 8.8m, GO III - IV, 1.60", 269.4deg, 1977). SB1
             (P = 2983d [09236]). Epoch of Min brightness is given.
             The deepest minima (corresponding to the middles of the
             descending branches of the radial velocity curve) are
             satisfied by the elements: Min = 2429355 + 2984d*E
             [01551].
mu    Gem    VB A (B 9.8m, 122", 141deg).
sig   Gem    VB A (B 10.8m, 182", 316deg); SB1 (P = 19.603d [09238]).
             There is a Min II on the light curve; Min II sometimes
             disappears and sometimes becomes deeper then Min I.
             Min II - Min I = 0.5P.
U     Gru    Depth of Min II 0.05m. d = 0.011P.
W     Gru    P var. Nonlinear term: +7.84d*10**(-9)*E**2. Min II 10.0.
X     Gru    d = 0.008P. Min II 10.69. P var.
             Current elements are given.
Z     Gru    Delta(S) = 12:.
             The shape of the light curve and P are strongly variable.
RS    Gru    (k - b)2 = 0.22.
RT    Gru    (k - b)2 = 0.02. Blazhko effect.
RV    Gru    (B - V)Max = +0.93. Min II 11.4.
RW    Gru    Delta(S) = 10. Blazhko effect.
RX    Gru    Min II 10.7.
RY    Gru    Superposition of irregular variations?
             During JD2434513 - 517 precalculated minima were not
             observed.
RZ    Gru    A description of light changes [02809].
UW    Gru    [Fe/H] = -1.6.
VW    Gru    P >= 260d?
VY    Gru    P > 160d.
VZ    Gru    RR type is also possible.
AK    Gru    Elements should be checked.
AP    Gru    P var. Mean elements JD2427992 - 36848 - see Table.
             during JD2434250 - 36848 Max = 2434337.337 + 0.5082945d*E.
AR    Gru    Min II 10.6.
AV    Gru    P >= 160d is possible.
AW    Gru    Min II? JD2436818.
BC    Gru    Min II 10.3. RRC type is possible.
BD    Gru    Min II 14.9.
BH    Gru    Min II 15.2:.
pi  1 Gru
             VB A (B 10.9m, G0V, 2.7", 202deg).
T     Her    VB A (B 10m, 67", 321deg).
U     Her    SiO, OH, H2O maser.
W     Her    ADS 10121 A (B 14.2m, 6", 334deg).
X     Her    P2 = 746d.
Z     Her    VB A (B ro > 10"). Min II 8.18.
             nonlinear term: -6.19d*10**(-10)*E**2.
RU    Her    SiO maser. The spectrum in Min
             light is composite; a companion? [03502].
RX    Her    Min II 7.74.
SW    Her    B - V; +0.12, +0.40. P var. Before 1921 Max =
             2416687.018 + 0.4928864d*E.
SX    Her    [Fe/H] = -1.8.
SY    Her    On period variations see [08699].
SZ    Her    Min II 10.10. P var. Min = 2430766.8390 + 0.818096d*E +
             0.0165d*sin(0.010465deg*E + 180deg) [05749].
             The Table gives current elements satisfac -
             tory after JD2438000.
TT    Her    Min II 9.89. The light curve shape var.
             P var. Before JD2430000 Min = 2425433.627 +
             0.9120846D [02389]; Min = 2434525.2572 + 0.9120800d*E
             (JD2430000 - 40000) [03504]; since JD2440000 - see Table.
TU    Her    d = 0.022P. P var. Before JD2435000 Min =
             2424381.416 + 2.2671303d*E - 854d*10**(-11)*E**2 [09240];
             Min = 2437462.3909 + 2.2669718d*E (JD2435000 -
             38000) [09241]; Min = 2443324.70097 + 2.2669385d*E
             (JD2438000 - 44000) [08593]; since JD2444000 - see Table.
TW    Her    [Fe/H] = -0.47.
TX    Her    Min II 8.97, DII = 0.11P. P var;
             periodic term: +0.0081d*sin(0.042deg*(E + 7255)).
UU    Her    [Fe/H] = -1.27.
             There was alternation of periods 90d and 71d
             [00310]; the period 45d [03507] was also noted.
             During JD2443611 - 44161 - see Table. Epoch of Min is given.
UX    Her    Min II 9.11. P var. Before JD2429000 Min =
             2419876.467 + 1.5488598d*E [00279]; Min =
             2429987.420 + 1.5488513d*E (JD2429000 - 38000)
             [03671]; since JD2438000 - see Table.
VW    Her    VB A (B 17.3m, 18", 120deg.
VX    Her    Delta(S) = 5. P var; nonlinear term:
             -0.00745d (E:10000)**2. According to [03369],
             a member of an eclipsing binary system.
VZ    Her    [Fe/H] = -0.9. P var. P = 0.44031880d (JD2415000 -
             22000) [05738]; Max = 2425004.4590 + 0.44032394d*E
             (JD2422000 - 27000); Max = 2425004.4456 +
             0.44032631d*E (JD2427000 - 36000) [03506];
             since JD2436000 - see Table.
WW    Her    VB A (B 15.6m, 7.4", 148.5deg, white).
WX    Her    Twice longer P is not excluded.
AC    Her    P var.
             The Table gives current elements valid since JD2442000.
             Mean P = 75.4619d [01754]. The magnitude in
             Max varies with Delta(m) = 1.6m [00368].
AD    Her    VB A (B 11.97m, 5", 189deg). d = 0.033P. Min II 9.79.
AF    Her    P var. Before JD2426950 P = 0.630336d;
             since JD2426950 - see Table.
             The shape of the light curve var.
AG    Her    P var. Max = 2422935.584 + 0.6494378d*E
             (JD2418210 - 26952); since JD2426952 - see Table.
AH    Her    Porb = 5.9d:. Oscillations during outbursts:
             24s <= P <= 39s, Delta(m) <= 0.003m [09251].
             Flicckering in Max And Min up to 0.4m in 2 - 8 minutes
             [09252].
AK    Her    ADS 10408 A (B 12.0m, 5", 323deg). Min II 8.64.
             Min II - Min I = 0.505P. dII = 0.07P. P var. Before
             JD2421200 Min = 2421200.549 + 0.42152207d*E; Min =
             2421200.549 + 0.42152083d*E (JD2421200 - 24950);
             Min = 2424949.555 + 0.42152061d*E  (JD2424950 -
             30000) [01760]; Min = 2430939.368 + 0.42152362d*E
             (JD2430000 - 41500); since 2441500 - see Table.
             The shape of the light curve var.
AM    Her    ‡U 1809 +50. Lx(soft)/Lopt ~15.
             Emissions of H and KCaII, H, HeI, HeII, etc.
             In the spectrum. Epoch of Min I in V light is given.
             The period shows complex variations. The phase of Min I
             in U light is 0.30p, in B 0.15P, in R 0.05P. Min I is
             probably due to an eclipse of a hot spot and the gas flow
             near the surface of the white dwarf by the white dwarf
             itself. The depth of Min I is up to 0.7m. Min II with the
             depth up to 0.4m (sometimes absent), Min II - Min I = 0.55P.
             Min II coincides  in phase with the X-ray eclipse.
             High and low states (b ~13.0m and B ~15.0m on average);
             in the high state there are variations with Delta(m) ~0.3m
             on the time scale >= 200d; the duration of low states is
             130d - 700d [09258] or less. During low states the
             depth of minima is small. Flickering up to 0.8mV in
             several minutes or dozens of seconds; X-ray flickering
             on the time scale of ~10s not correlating with
             optical flickering. The magnetic field ~1*10**7 G at
             the equator, ~2*10**7 G on poles. Variable circular
             (from  +3% to -9%) and linear (up to 7%) polarization.
             IR excess at lambda 10 mkm.
AP    Her    P var strongly. P = 10.400d (JD2415000 -
             19000:); P = 10.3970d (JD2423700 - 24700:); P =
             10.4260d (JD2424700 - 25300); P = 10.4338D
             (JD2425800 - 27000); P = 10.3945d (JD2427000 - 27400);
             P = 10.4277d (JD2433000 - 33850); P = 10.3898d
             (JD2433850 - 34850);  P = 10.4209d (JD2434850 - 35600);
             P = 10.3715d (JD2435600 - 37200);
             DURING JD2437200 - 43800 - see Table.
             The light curve shape var. [A/H] = -0.8.
AR    Her    P var in a complicated way. Max =
             2424794.274 + 0.4700234d*E (1905 - 1954) [06535];
             Max = 2439692.683 + 0.469975d*E (1954 - 1967) [05274];
             since 1967 - see Table.
             Blazhko effect, Pi = 31.5489d [03555],
             Delta(m) var (0.9m -: 1.8m pg) [02168], (M - m) var.
             Delta(S) = 6.
AT    Her    The star is bright on one plate (JD2418209).
             Besides that, 11.8m - 12.25m.
AW    Her    VB A (B 10" - 20"). d = 0.03P.
BB    Her    P var. P = 7.507696D (JD2418924 - 30700);
             since JD2430700 - see Table. [A/H] = +0.3.
BC    Her    P var. Before JD2432000 Min = 2426242.372 +
             3.08752d*E [09262]; since JD2436000 - see Table.
BD    Her    P var. P = 0.4739135d (JD2426540 - 29620); P =
             0.4739057d (JD2429620 - 30570); Max = 2430495.404 +
             0.4739126d*E (JD2430570 - before 1948) [09263];
             since 1948 - see Table. Delta(S) = 0.8.
BL    Her    P var. P = 1.3074604d (JD2415000 - 35000);
             since JD2435000 - see Table. Another possible
             representation: Max = 2434999.402 + 1.307457d*E -
             3.9d*10**(-10)*E**2 (JD2415000 - 42000). [Fe/H] = 0.0.
BO    Her    d = 0.015P. Min II 10.8. P var?
CC    Her    P var. Min = 2426120.415 + 1.7340314d*E (JD
             2425790 - 31265); Min = 2431265.288 + 1.7340460d*E
             (JD2431265 - 36000) [02389]; Min = 2439668.342 +
             1.73398d*E (JD2436000 - 39600); since JD2439600 - see
             Table.
CD    Her    The chart in [06286] is wrong.
CE    Her    [A/H] = -1.8.
CK    Her    P var? Max = 2429231.234 + 0.519201d*E (JD2429231 -
             877) [00332]; during JD2436041 - 37955 - see Table.
CO    Her    P2 = 600d. Sometimes does not vary for 150d.
CP    Her    Superimposed waves, 50d - 100d.
CT    Her    The depth of min II 0.05m. P var.
             Min = 2430904.431 + 1.786337d*E (JD2426480 - 35000)
             [03567]; Min = 2439355.666 + 1.7863645d*E
             (JD2435000 - 39500) [00001]; Min = JD2441499.3307 +
             1.7863891d*E (JD2439500 - 42500) [08593];
             since JD2442500 - see Table.
DE    Her    P var. Max = 2425754 + 171.2d*E (JD2425754 - 30890);
             Max = 2430889 + 175.3d*E (JD2430890 - 36150);
             during JD2436150 - 38140 - see Table.
DF    Her    Elements are valid since JD2425900.
DH    Her    d = 0.024P:. Min II 9.5.
DI    Her    Min II 8.95, DII = 0.03P, Min II - Min I = 0.77P (1966 -
             1978). Apsidal motion: P = 29000yr +- 4000yr;
             Min II = 2442241.4602 + 10.5501751d*E.
             A considerable discrepancy between the observed and
             the theoretical rate of apsidal motion.
DK    Her    P var.
DL    Her    Blazhko effect, Pi = 33.6d, 11.0m <= m Max <= 11.3m. P var.
             Delta(S) = 5.
DO    Her    Close to V362 Her.
DQ    Her    VB A (B 18.17m, F, 3.5", 132deg, optical?).
             Nebula, R = 10.5" (Halpha, 1981).
             After the main Max of the Nova a deep
             Min 13.0m (JD2426925) and a flat secondary Max
             6.7m (JD2427065) were observed.
             Eclipsing variability:
             14.61m - 18.08m, Min HeI = 2434954.9445 + 0.193620877d*E
             [09280]. D = 0.20P, d = 0.000P.
             The light curve shape and Delta(M) var.
             Oscillations: Max HeI = JED2434954.785868 +
             8.22521640d*10**(-4)*E - 2.8048d*10**(-16)*E**2
             [08722], 0 <= Delta(m) <= 0.08m.
             Polarization changes with double oscilation period.
             Flickering: Delta(m) = 0.15m.
DY    Her    P var, nonlinear term: -18.6d*10**(-13)*E**2.
EI    Her    Red.
EN    Her    P var. Before JD2427000 P = 160d.
ES    Her    Min II 13.7.
ET    Her    The elements are valid earlier than JD2427200
EX    Her    Red.
EZ    Her    The elements are valid earlier than JD2427400.
FN    Her    P var?
FW    Her    Min II 14.6.
FY    Her    According to the spectrum, EW type is possible.
GL    Her    P var?
GU    Her    d = 0.010P. Min II 11.8. Min II - Min I = 0.513P.
GV    Her    [Fe/H] = -1.41. P var. Max = 2427543.360 +
             0.2914606d*E (JD2427543 - 29728) [00152];
             during JD2436041 - 38170 - see Table.
GY    Her    P var. Max = 2428219.623 + 0.524347d*E (JD2428219 -
             727) [00152]; during JD2436370 - 38170 - see Table.
HS    Her    d = 0.025P. Min II 8.63. P var; since JD2438240 - see
             Table. Apsidal motion: Pi ~130yr [06538].
HV    Her    d = 0.008P:; Min II 12.9:.
HZ    Her    Her X-1 = 4U 1656 + 35. Lx/Lopt = 2 - 60.
             The Table gives elements for light minima due
             to eclipsing variability and the reflection effect. Min I
             coincides with the X-ray eclipse. Shallow Min II may
             be present. The reflection effect causes variations
             with Delta(m) up to 1.5m. A cycle of 34.875d duration is
             observed in X-ray band; the source is faint during
             two thirds of the cycle. The optical light curve changes
             are observed during the 35d cycle [09283]. According to
             [06539], during JD2427543 - 657 and JD2428630 - 29789 the
             strong reflection effect was absent; the star was still
             varying with P = 1.7d and had Delta(m) ~0.5m,
             Min I = Min II. In [06546] it is stated that
             such intervals with no reflection effect, of 8d to 7a
             duration, took place for almost half the time since
             1890. The light changes during such intervals are in
             the range 14.7m - 15.2m pg. Since 1957 intervals without
             the reflection effect were not observed. In June - July
             1983 the predicted phases of high X-ray flux
             did not take place, but the reflection effect did not
             disappear [09284]. Secondary light variations: P1 =
             1.0977d (delta(B1) = 0.33m), P2 = 0.871173d*E
             (delta(B2) = 0.10m),
             P3 = 1.623846d*E (delta(B3) = 0.17m) [09285]. X-ray pulsar,
             P = 1.2377991s (JD2443357), dP/dt/P = (-2.9 +- 0.2)*10**(-6)/yr
             [09286], sometimes noticeable also in the
             optical range [06543]. Rapid brightness flickering.
IK    Her    d = 0.030P?
IQ    Her    Superposition of variations with shorter P and
             small Delta(m) [06645].
IT    Her    According to the spectrum, EW type is possible.
KL    Her    Min II 14.7.
KV    Her    The light curve is characteristic of Mira Ceti stars
             but strongly varies. Many irregularities. O - C: -96d, +73d.
LR    Her    Min II 15.4:.
LS    Her    The light curve shape var.
LT    Her    d = 0.02P. Min II 10.79.
LV    Her    P var? During JD2428429 - 31342 - see Table.
MM    Her    VB A (B 13.50m, 18", 120deg). Min II 9.7.
             Delta(m) of the distorsion wave up to 0.12m.
MP    Her    [Fe/H] = -1.18.
MS    Her    Min II 13.3.
MT    Her    Min II 12.30.
MV    Her    The chart in [00156] identifies the variable erroneously;
             real MV Her is marked as "C".
MW    Her    P var. P = 503d (1976) [09290]. During
             JD24668 - 29172 - see Table.
MX    Her    Moments of Min after JD2444000 published by different
             groups of observers contradict each other.
NQ    Her    According to [03882], EA, 8.0 - 8.6 pg, Min II
             8.4, Min I = 2426894.433 + 0.870218d*E (JD2426894 - 34250).
NR    Her    Waves, P = 2.8d - 5.5d.
OQ    Her    Epoch of min is given.
OS    Her    B - V: +0.12,  +0.48.
OU    Her    Spectral type is given according to [02198]; in BSD-G7.
OX    Her    Delta(S) = 6:.
PW    Her    Min II 10.1; DII ~0.3P(!).
V0338 Her    Min II 10.13. P var. Before JD2437000 Min =
             2433771.38 + 1.305732d*E [03115]; Min = 2441864.379 +
             1.3057515d*E (JD2437000 - 43400) [08593, 00001];
             since JD2443400 - see Table.
V0342 Her    Min II 10.7.
V0347 Her    P var. Max = 2415288.21 + 0.5373619d*E (JD2415288 -
             18596); since JD2429495 - see Table.
V0359 Her    P var. Min = 2416046.476 + 1.755754d*E (JD2416000 -
             26500) [00001]; Min = 2435693.47 + 1.755775d*E (JD
             2426500 - 36000) [01040]; since JD2443500 - see Table.
V0362 Her    Close to DO Her.
V0365 Her    Blazhko effect: Pi = 40.64d. P var.
             During JD2429037 - 36840 - see Table.
V0373 Her    P = 0.33d or 0.50d is possible.
V0384 Her    P ~0.33d is possible.
V0387 Her    Min II 13.2.
V0394 Her    P var?
V0395 Her    Z = 0.0643.
V0396 Her    Z = 0.175.
V0403 Her    Min II 16.0:.
V0412 Her    Min II 15.2.
V0422 Her    P var? During JD2434131 - 35991 - see Table.
V0423 Her    Min II 15.0.
V0426 Her    Min II 15.8.
V0431 Her    P var.
V0436 Her    The elements are uncertain.
V0441 Her    IR excess, evidence for a circumstellar envelope. Possibly
             non-radial pulsation.
V0442 Her    P var. Max = 2434223.375 + 0.4421143d*E (JD2417447 - 36083);
             since JD2435730 - see Table.
             The shape of the light curve varies.
V0446 Her    Before the outburst 16.2m - 18.8m [03607].
V0451 Her    ADS 10310 A (B 10.70m, 19", 239deg).
             The epoch of Min U light is given.
V0458 Her    [Fe/H] = -1.65.
V0463 Her    P = 54.4d is possible.
V0477 Her    Min II 15.4.
V0482 Her    Possibly eclipsing.
V0499 Her    Blazhko effect.
V0502 Her    Min II 13.5?
V0510 Her    P var?
V0511 Her    P var?
V0513 Her    Min II 15.7.
V0516 Her    Min II 17.1.
V0523 Her    Elements are valid during JD2430940 - 990.
V0524 Her    Twice shorter P is possible.
V0527 Her    Max = 2430938.451 + 0.5188d*E (JD2430938 - 990);
             during JD2436308 - 318 - see Table.
V0529 Her    Epoch of Min is given.
             According to [04217], P = 120d.
V0533 Her    VB A (B 16m, 9.5", 0deg). oscillations:
             Max = 2443717.730281 + 0.0007364941d*E, A ~1% [04162].
V0551 Her    P = 4.00d/n is possible.
V0552 Her    P = 3.04d/n is possible.
V0554 Her    P = 4.01d/n is possible.
V0557 Her    P = 8.00d/n is possible.
V0570 Her    P = 0.5d or 0.33d is possible.
V0578 Her    Red.
V0582 Her    VB. Red.
V0583 Her    Red.
V0588 Her    Possibly eclipsing.
V0600 Her    SB, Porb - see Table. Variability of Vr possibly caused by
             BCEP type pulsations: P - 0.18d.
V0601 Her    Elements are valid since JD2439184.
V0604 Her    Red.
V0608 Her    Blazhko effect.
V0615 Her    Red.
V0618 Her    P var?
V0624 Her    VB A (12.04m, 40"). Min II 6.35. SB2.
V0637 Her    ADS 10227 A (BC 9.2m, 9.2m, 1.7", 18deg, 1975; BC: A =
             0.28", Porb = 56.56yr).
V0639 Her    mu alpha = -0.21", mu delta = +0.39",pi = 0.087".
             VB B (A = V647 Her, 11.36m var, dM4e; B 16", 268deg).
             Flares in the bands U and M pg.
V0640 Her    VB A (B 14.9m, 8.5", 217deg; C 13.9m, 23", 221deg).
V0641 Her    L or ISB type is also possible.
V0644 Her    SB (Porb = 11.859d).
V0645 Her    P ~3h - 10h, a cycle of 40d.
V0647 Her    VB A (B = V639 Her, 16", 268deg); mu alpha = -0.21",
             mu delta = +0.39"; pi = 0.087".
V0652 Her    P var; nonlinear term: -45.80d*10**(-10)*E**2. Delta(m) var.
             Resembles PV TEL type stars but is a helium rich subdwarf.
             Epoch of Max is given. Secondary hump at the phase 0.5P.
V0654 Her    Delta(m) = 0.15m in white light.
V0655 Her    ADS 10407 A (B 9.2m, 4.1", 144deg, 1971).
V0657 Her    According to [02610], CST?, 11.0m.
V0662 Her    Less probable P values: 0.56629d, 0.56710d, 0.56881d,
             0.56970d.
V0685 Her    Min II 15.8.
V0687 Her    Min II 14.9.
V0691 Her    Possible P values: 0.927d, 0.637d.
V0697 Her    H2O, OH maser.
V0699 Her    Min II 16.0:.
V0717 Her    Blazhko effect?
V0718 Her    Min II 14.3.
V0719 Her    EW type with twice longer P is not excluded.
V0720 Her    Blazhko effect?
V0721 Her    Blazhko effect?
V0722 Her    Min II 15.7.
V0723 Her    Min II 15.5.
V0728 Her    Min II 11.4.
V0731 Her    Min II 13.8.
             Twice shorter P is not excluded.
V0732 Her    Min II 13.8.
V0733 Her    Min II 14.3:.
V0737 Her    Blazhko effect?
V0740 Her    Min II 14.4.
V0741 Her    Blazhko effect?
V0742 Her    Min II 14.4.
V0744 Her    Vr var, P = 86.7221d (SB1? nonradial pulsatiob?).
             Rapid spectral variability is possible: P = 2.5552d,
             0.78906d.
V0749 Her    P = 465s.
V0771 Her    Epoch of max U light is given.
V0772 Her    VB AB (7.4m, G0V; 8.5m, G8V:; A = 0.27", E = 0.97, P =
             20.0yr, C 10.62m, 28"). One of the components
             (probably B) is SB1, P = 0.879511d [04056]. The same
             component must be the eclipsing system. Faint X-ray
             source.
V0774 Her    Both flares and "antiflares" (abrupt fadings) of
             comparable amplitude are observed.
V0946 Her    Not Wolf 688, a large-proper-motion star, which is at 17h19m28s.9,
             +33deg05'10" (epoch and equinox 2000.0).
V0973 Her    Suspected rapid brightness variations.
V0994 Her    The secondary component of the double system may also vary.
alf   Her    ADS 10418 A (B 5.39m, 4.9", 107deg, 1973; B - SB2,
             G5III + F2V). Slow variations, P ~6yr, Delta(m) ~0.5m;
             quicker changes, P ~ 50d - 155d, Delta(m) ~ 0.3m - 1.0m.
             Together with the visual companion the
             star is surrounded by an enormous envelope (R ~2*10**5R$,
             expansion velocity 10 km/s, mass loss 3*10**(-8)M$/yr).
nu    Her    [Fe/H] = -0.26. SB?
omi   Her    VB interferometric.
phi   Her    SB, Porb = 560.5d.
ome   Her    ADS 10054 A (B 11.5m, 0.8", 232deg, 1967; C 11.0m, 28.4",
             96deg, 1957; D 27.5", 271deg, 1960). Epoch of Min is given.
             Double wave in the light curve.
             Rapid variations, P = 0.15d [09310].
g     Her    The mean cycle 1972 - 1981 is given. Slow pulsations
             (<P> = 875d +- 70d) and non-periodic variations on the
             time scale of 5d - 15d with Delta(m) up to 0.2m are
             superimposed.
u     Her    ADS 10449 A (B 10.2m, 4.4", 60deg). Min II 4.93.
R     Hor    OH, H2O, SiO maser. P var. Max = 2428868 + 401.5d*E
             (JD2412800 - 28900); since JD2428900 - see Table.
V     Hor    <P> = 59d (JD2428380 - 910), <P> = 90d (JD2429170 - 980).
X     Hor    Epoch of Min brightness is given. Maxima are broad.
             Usually secondary minima are observed.
SY    Hor    Min II 12.0.
SZ    Hor    Min II 10.7:.
TU    Hor    Min II 6.03; Min II - Min I = 0.52P;
             Max II is fainter than Max I by 0.05m. Peculiar
             ellipsoidal variable [09245].
TY    Hor    Type RCB?
UU    Hor    P var. Max = 2416826.417 + 0.6436900d*E (JD2416800 - 25000);
             since JD2425000 - see Table.
UX    Hor    Min II 14.4. P var. Min I = 2426659.380 + 0.7126943d*E
             (JD2426650 - 30860); since JD2430540 - see Table.
UZ    Hor    P var. Max = 2426679.425 + 0.338188d*E (JD2426300 - 28430);
             since JD2430040 - see Table.
VY    Hor    mu = 0.173", ro = 33deg. P = 314s, 617s.
R     Hya    VB A (B 13.0m, 21.6", 324deg). SiO maser. P var. According
             to [00458]; Max = 2328201 + 486d*E (JD2328200 - 31120);
             Max = 2343512 + 507d*E (JD2343300 - 44800);
             Max = 2372678 + 485d*E (JD2372200 - 72700);
             Max = 2380447 + 477d*E (JD2380000 - 81400);
             Max = 2385160 + 461d*E (JD2384700 - 88000);
             Max = 2394350 + 448.6d*E (JD2393900 - 2402000);
             Max = 2403742 + 434d*E (JD2403300 - 04200);
             Max = 2406363 + 429.5d*E (JD2406000 - 11100);
             Max = 2413642 + 411d*E (JD2413200 - 14100);
             Max = 2416563 + 405.5d*E (JD2416100 - 23400);
             Max = 2424288 + 414.7d*E (JD2423400 - 28500).
             since JD2428500 - see Table.
T     Hya    P var. Max = 2399455 + 289.00d*E(JD2398600 - 2421700);
             Max = 2422584 + 294.2d*E (JD2421700 - 25800);
             Max = 2431781 + 284.20d*E (JD2425800 - 36200); since
             JD2437500 - see Table.
V     Hya    VB A (B 11.58mV, KO III, 46", 186deg).
             Mean brightness variations with P = 6670d and A = 3.5m are
             superimposed by light oscillations with A = 1.1m - 2m and
             elements given in the Table. Deep light minima were
             observed in 1891, 1908, 1925, 1942 - 43, 1959,  and 1962.
             A graph of the light curve [03614].
W     Hya    VB A (B 9.3m, 72", 108deg). P var. Max = 2411074 + 379d*E
             (JD2411000 - 14150); Max = 2414644 + 395d*E
             (JD2414150 - 19400); Max = 2419746 + 378d*E
             (JD2419400 - 25200) [00458]. Max = 2425740 + 366d*E
             (JD2425200 - 27000); Max = 2440336 + 397.35d*E
             (JD2428000 - 40500); since JD2440500 - see Table.
             Amplitude and shape of the light curve vary strongly.
             OH, H2O, SiO maser.
X     Hya    OH, H2O, SiO maser.
Y     Hya    Mean magnitude varies.
RR    Hya    H2O maser.
RS    Hya    P var. Max = 2422973 + 330.2d*E (JD2414000 - 23000);
             Max = 2429126 + 342.0d*E (JD2423000 - 29200); Max =
             2429455 + 331.2d*E (JD2429200 - 34500);
             since JD2434500 - see Table.
RT    Hya    Before 1952 <P> = 255d; since 1952 - see Table.
             The character And amplitude of light variations vary
             strongly.
RU    Hya    OH, H2O maser. P var. Max = 2429572 +
             334.0d*E (JD2414000 - 29600); since JD2428500 - see
             Table.
RW    Hya    SB2 (P = 370d). Epoch of Min brightness is given.
RX    Hya    VB A (B 10.5m). Depth of Min II 0.05m. P var.
             Min I = 2428261.385 + 2.2815942d*E (JD2419500 -
             28500); Min I = 2440650.409 + 2.2816200d*E
             (JD2428500 - 41400); since JD2441400 - see Table.
SS    Hya    VB A (B 12.0m, 13", 195deg); SB2.
SU    Hya    Mean magnitude varies with P = 780d.
SV    Hya    VB A (B 35", 225deg). Delta(S) = 7.
SX    Hya    D = 0.022P. P var. Min I = 2427659.223 + 2.895697d*E
             (JD2410000 - 28000) [00007]; since JD2442500 - see Table.
SY    Hya    P var. Min = 2425590.589 + 3.403082d*E (JD2425500 -
             31150) [07548]. Since JD2432200 - see Table.
SZ    Hya    P var. Max = 2415714.1429 + 0.53742815d*E
             (JD2414700 - 26500) [03626]; Max = 2426410.575 + 0.53736d*E
             (JD2426400 - 27200) [00001]; Max = 2431881.5537 +
             0.53723051d*E (JD2427880 - 35200) [03626]; Max =
             2435542.267 + 0.5372497d*E (JD2435500 - 38900)
             [03627]. Since JD2438770 - see Table.
             Blazhko effect: Max(A) = 2440705 + 25.8d*n [06557];
             10.44m <= Max <= 11.03m.
TT    Hya    Min II 7.32; d = 0.035P.
TU    Hya    P var. Max = 2416980 + 277.5d*E (JD2412500 -
             17300); Max = 2417260 + 272.5d*E (JD2417200 -
             19800) [01787]; Max = 2430410 + 281.4d*E
             (JD2420500 - 30500); Max = 2438332 + 272.3d*E
             (JD2432000 - 39200); since JD2439200 - see Table.
TY    Hya    P var. Min = 2434478.464 + 4.660978d*E (JD2419800 -
             35000) [01788]; since JD2435000 - see Table.
UU    Hya    P var. Max = 2427423.84 + 0.5238585d*E (JD2414950 - 27400)
             [01789]; Max = 2429729.835 + 0.523854d*E (JD2427000 - 31000)
             [00752]. Spectrum is based on Ca II.
UW    Hya    Min II 13.8:; Min II - Min I = 0.64P. P = 1.055439d?
UY    Hya    Min II 13.8. RRC?
VV    Hya    P var. Max = 2427421 + 155d*E (JD2419500 - 37000)
             [01792]; since JD2437000 - see Table.
VX    Hya    (k - b)2 = 0.26.
             Luminosity class [03149] contradicts the type of light
             variability. The shape of the light curve strongly varies.
             The main oscillation with the period P0 given in the Table
             is superimposed by the secondary one with P1 = 0.172720d
             [03631]. P1/P0 = 0.773; Pb = 0.761445d.
VY    Hya    Min II 9.1.
VZ    Hya    Min II 9.46.
WY    Hya    Min II 11.2.
WZ    Hya    (k - b)2 = 0.06. P var. Max = 2416169.681 + 0.53772640d*E
             (JD2414000 - 19000); Max = 2419811.736 +
              + 0.53775858d*E (JD2419000 - 21000); Max =
              = 2424618.630 + 0.53774101d*E (JD2421000 - 32000)
             [00752]; Max = 2436613.445 + 0.5377229d*E
             (JD2436600 - 38500) [03633]; since JD2438000 - see Table.
XX    Hya    P var. Max = 2439560.355 + 0.50774868d*E
             (JD2428200 - 39560) [05238]; since JD2439560 - see Table.
XZ    Hya    Min II 15.0.
AE    Hya    Min II 14.6.
AF    Hya    Min II 13.8.
AI    Hya    Min II 9.84; Min II - Min I = 0.438P; DII = 0.075P;
             dI = 0.02P; dII = 0.00P; EA/DM. Pulsation
             period P' = 0.13803d, A = 0.02m - 0.03m [09259].
AV    Hya    Min II 10.35; dI = 0.023P:.
CH    Hya    Min II 15.5; Min II - Min I = 0.57P.
CO    Hya    Found in Lupus, in 10deg to the south from the position
             published by the discoverer [00078].
CW    Hya    P var? [04027].
             Elements given in the Table satisfy observations only in
             the interval JD2428950 - 30375.
DD    Hya    P var. Max = 2431139.313 + 0.501818d*E (JD2431100 -
             600) [01432]. Since JD2441600 - see Table.
DE    Hya    d = 0.014P?
DF    Hya    Min II 11.5.
DH    Hya    Delta(S) = 7.
DK    Hya    Min II 10.7.
DM    Hya    d = 0.15P?
EU    Hya    Min II 10.2.
EX    Hya    Light variations with Porb and amplitude up to 0.9mV
             due to eclipses of hot spot are represented by the
             elements: ET(Min) = 2437699.94177 + 0.0682338422d*E,
             where ET(Min) is the heliocentric Julian Date converted
             to Ephemeris Time; simultaneously periodic modulation of
             the shape of the light curve between the outbursts is
             observed with the amplitude 0.2m - 0.9m and the elements:
             Max = 2437699.8895 + 0.04654656d*E - 1.2d*10**(-12)*E**2
             [09265]. Mean interval between bright outbursts is 465d
             [05695], mean cycle is close to 20 - 30d.
EY    Hya    P var. Max = 2432707 + 160.5d*E (JD2426100 - 32800);
             since JD2432800 - see Table.
EZ    Hya    Min II 10.7. P var. Min I = 2440255.8482 + 0.44976658d*E
             (JD2431160 - 40650) [07549]; since JD2440250 - see Table.
FG    Hya    Min II 10.25; dI = dII = 0.085P. P var. Min I =
             2431150.388 + 0.3278422d*E (JD2431140 - 34400)
             [00182]; Min I = 2436968.7067 + 0.32783433d*E
             (JD2434050 - 400) [03639]; Min I = 2436968.7067 +
             0.32783546d*E (JD2436950 - 43250) [09267];
             since JD2444600 - see Table.
FI    Hya    V27 in the globular cluster NGC 4590
             (M68); cluster non-member.
FS    Hya    According to [01480] P = 91.7d.
FW    Hya    Min II 12.4.
FY    Hya    VB A (B 15.45m, 15", 90deg); Delta(S) = 7:; (k - b)2 = -0.03.
GK    Hya    Min II 9.57.
             There is a square term in the elements:
             -4.01d*10**(-9)*E**2.
GM    Hya    d <= 0.01P.
GN    Hya    Min II 13.6.
GT    Hya    Cep?
HS    Hya    Min II 8.55.
IK    Hya    Blazhko effect with Pi ~30d.
IW    Hya    OH, H2O maser.
KM    Hya    P var?
KU    Hya    VB AB (7.3m, 7.4m, A = 0.150", P = 58.93 yr, E = 0.219);
             A(v) = 0.06m.
KW    Hya    Porb = 7.75043d; E = 0.110 [09273]; Min II 6.35;
             Min II - Min I = 0.54P.
bet   Hya    VB A (B 5.6m, 0.9", 8deg, 1959).
khi 2 Hya    Min II 5.92.
Y     Hyi    d = 0.024P.
RR    Hyi    In the constellation Octans.
RS    Hyi    In the region of the Small Magellanic Cloud.
             Not a member of the cloud.
RT    Hyi    Min II 14.1.
RV    Hyi    Min II 12.4; Min II - Min I = 0.61P.
RY    Hyi    In the region of the Small Magellanic Cloud. Not a member
             of the Cloud.
ST    Hyi    The member of the Small Magellanic Cloud. [A/H] = -0.8.
SZ    Hyi    In the region of the Small Magellanic Cloud. Not a member
             of the Cloud.
TW    Hyi    Delta(S) = 10:.
UU    Hyi    P = 112.25d?
VW    Hyi    Mean interval between the supermaxima is 179d.
             Porb = 0.0742711d. Between the normal outbursts the
             brightness periodically increases by 0.35m - 0.40m because
             of hot spot appearances:
             Max = 2440128.0222 + 0.0742711d*E [07550]. During the
             supermaxima the period between the superhumps is
             0.0769d [09275]. Sometimes the light oscillations with
             the amplitude 2% and cycle from 28s to 34s are observed
             [07551].
VY    Hyi    In the region of the Small Magellanic Cloud. Not a member
             of the Cloud.
VZ    Hyi    RR [00193].
WX    Hyi    Mean interval between the supermaxima is 141.5d.
             Porb = 0.0748134d [09277]. Period between the superhumps
             observed during the supermaxima is 0.07737d [09278].
WZ    Hyi    In the region of the Small Magellanic Cloud. Not a member
             of the Cloud.
ZZ    Hyi    A galaxy PGC 232232 [00001].
AC    Hyi    In the region of the Small Magellanic Cloud. Not a member
             of the Cloud.
BB    Hyi    Delta(S) = 7:.
V     Ind    P var. Max = 2439792.276 + 0.4796030d*E
             (JD2414000 - 40000) [05233]; since JD2440000 - see Table.
             Delta(S) = 7, (k - b)2 = 0.02.
RS    Ind    Min II 10.0. P var.
RU    Ind    VB A (B 12.6m, 2.3", 103deg). Min II 12.1.
RX    Ind    240d < P < 310d.
RY    Ind    Min II 11.04.
ST    Ind    Min II 11.79.
SU    Ind    Min II 9.5:.
TV    Ind    Min II 11.9.
AR    Ind    Min II 14.4. RRC?
AY    Ind    mu alpha =  +0.345", mu delta = -0.310"; VB?
R     Lac    VB A (B 14.1m, 6", 50deg).
S     Lac    P var. Max = 2412857 + 238.2d*E (JD2410000 - 16400);
             Max = 2418828 + 241.45d*E (JD2416400 - 20500); Max =
             2427307 + 242.7d*E (JD2420500 - 27300); Max =
             2437290 + 237.4d*E (JD2427300 - 37300);
             since JD2437300 - see Table.
U     Lac    There are light variations with the periods:
             150d, 550 - 690d, 2900d.
V     Lac    P var. There is a square term in the elements:
             -6.48d*10**(-8)*E**2.
W     Lac    P var. Max = 2415255 + 323d*E (JD2414600 - 15300);
             Max = 2425628 + 335.5d*E (JD2425600 - 38000) [00458];
             Max = 2433844 + 324.5d*E (JD2428000 - 33850);
             since JD2433850 - see Table.
X     Lac    P var. Max = 2418890.497 + 5.444303d*E (JD2416670 -
             29500) [02033]; since JD2429500 - see Table.
Z     Lac    P var. There is a square term in the elements:
             -3.4d*10**(-8)*E**2. [A/H] = 0.2.
RR    Lac    P var. Max = 2419434.331 + 6.416146d*E (JD2417900 - 31600);
             since JD2431600 - see Table. [A/H] = 0.0.
RT    Lac    Min II 9.62. P var. Min I = 2440382.9005 + 5.0740484d*E +
             1.02d*10**(-8)*E**2 (JD2411650 - 42500) [08592];
             since JD2436470 - see Table.
             There is a square term in the elements given in the Table:
             -2.7d*10**(-8)*E**2. Shape of the light
             curve and depths of the Minima vary. According to
             [09293] the period of the distortion wave migration is
             ~9.5 yr, the period of the wave amplitude variations
             (0 < A <= 0.17m) is ~30 yr. According to [09292] the
             migration period is nearly half of the value given in
             [09293].
RV    Lac    Mean magnitude varies with the period 550 - 700d.
RW    Lac    Min II 10.8; DII = 0.024P; Min II - Min I = 0.492P.
RX    Lac    S7.5/1e. P = 174d (JD2414950 - 29550) [01026];
             since JD2436800 - see Table.
RY    Lac    Oscillations of mean magnitude with P = 300 - 420d
             and A <= 0.5m are superimposed by oscillations with
             P = 38 - 91d.
SS    Lac    Probable member of the open cluster NGC 7209. Min II 10.5;
             Min II - Min I = 0.57P; d = 0.008P.
             Apsidal motion with P = 1000 yr is possible.
ST    Lac    Elements should be checked.
SU    Lac    P var. Max = 2412748 + 279.10d*E (JD2412700 - 27000)
             [05707]; Max = 2426972 + 286.74d*E (JD2426900 - 31000);
             Max = 2431008 + 306.0d*E (JD2431000 - 33150)
             [00001]; Max = 2433150 + 319.14d*E (JD2433150 - 42150)
             [05707]; since JD2442100 - see Table.
SW    Lac    Min II 9.31. P var. Min I = 2418943.712 + 0.32071236d*E
             (JD2410000 - 19990); Min I = 2420038.621 +
             0.32071510d*E (JD2419990 - 25210); Min I =
             2430996.525 + 0.32071665d*E (JD2425210 - 33690);
             Min I = 2436046.5634 + 0.32072132d*E (JD2433690 - 36755)
             [05222]; Min I = 2437572.5723 + 0.32072811d*E
             (JD2436755 - 40000) [03374]; Min I = 2440467.4592 +
             0.32072480d*E (JD2440110 - 40500) [06089]; Min I =
             2441249.3737 + 0.3207197d*E (JD2440500 - 41600);
             [00001]; Min I = 2442697.4039 + 0.3207144d*E
             (JD2441600 - 43100) [09295]; Min I = 2443459.7476 +
             0.3207216d*E (JD2443100 - 44400) [09297]; Min I =
             2444856.8064 + 0.3207184d*E (JD2444400 - 44900)
             [00001]; since JD2444900 - see Table.
             Shape of the light curve, depths of minima and heights
             of maxima vary.
TW    Lac    d = 0.018P. P var. Min I = 2424387.332 + 3.0374936d*E
             (JD2424380 - 34000) [02389]; Min I = 2434049.593 +
             3.037520d*E (JD2434000 - 36560) [03115];
             since JD2441500 - see Table.
TZ    Lac    In the region of the open cluster NGC 7243.
UW    Lac    Depth of Min II 0.05m; d = 0.028P. P var.
             Min I = 2429158.17 + 5.2902d*E (JD2414580 - 29440)
             [01813]; Min I = 2429158.17 + 5.290000d*E
             (JD2429440 - 35800) [03115]; since JD2436800 - see Table.
             Apsidal motion is possible [09300].
UY    Lac    d = 0.022P.
UZ    Lac    P var?
VX    Lac    P var. Min = 2424791.488 + 1.0744891d*E
             (JD2424700 - 32400); Min = 2432479.477 + 1.0744991d*E
             (JD2432400 - 40510); Min = 2440750.971 +
             1.0744881d*E (JD2440750 - 43000) [07552];
             since JD2443000 - see Table.
VY    Lac    Min II 10.6. P var? Min I = 2434629.392 + 1.036245d*E
             (JD2424700 - 39830) [01804]; since JD2440080 - see Table.
WY    Lac    Light variations with P = 850d and A = 1.5m are
             superimposed by variations with P = 50d and A = 1m.
XX    Lac    In the region of the open cluster NGC 7243.
XZ    Lac    P var.
AG    Lac    Min II 14.0.
AR    Lac    Min II 6.43; Min II - Min I = 0.5018P; dI = 0.045P; DII =
             0.13P; dII = 0.00P. P var. Min I = 2426624.378 +
             1.983244d*E (JD2415300 - 26800) [09309]; Min I =
             2429535.739 + 1.9832125d*E (JD2426800 - 36000)
             [09312]; Min I = 2437018.414 + 1.983252d*E
             (JD2436000 - 37500) [00001]; since JD2437500 - see Table.
             There is a square term in the elements
             given in the Table:  - 5.24d*10**(-9)*E**2.
             Shape of the light curve varies; there is a
             distortion wave with A up to 0.13mV migrating in the
             direction of decreasing phases with P ~2.5 yr. Spectrum
             investigations [01816, 09315, 9316].
AU    Lac    Min II 12.2; Min II - Min I = 0.53P.
AW    Lac    Min II 11.2.
BH    Lac    Hydrogen lines in the spectrum are sharp and deep [03149].
BL    Lac    Z = 0.07; <B-V> =  +1.0. Light curve graph [06784].
BM    Lac    The elements are valid in the interval JD2425200 - 26250.
BT    Lac    There is a square term in the elements: -0.0004d*E**2.
             Epoch of Max brightness is given in the Table.
             Mean brightness varies in the range 13.8m - 15.2m with
             P = 654d. Mean amplitude of the shortperiodical variations
             is ~1.5m. There occur changes of primaries and
             secondaries minima into each other.
BU    Lac    The main variation is superimposed by waves with a
             possible period -200d.
CG    Lac    Min II 14.0.
CM    Lac    Min II 8.53; DII = 0.12P.
CN    Lac    Min II 12.6. In the region of the
             open cluster NGC 7209. Not member of the cluster.
CO    Lac    Min II 10.79. Apsidal motion with
             P = 42.3 yr is observed. There is a periodic term in
             The elements given in the Table: -0.0133d cos(157.7deg +
             0.0359deg*E). Min II = 2427534.8439 + 1.5422075d*E +
             0.0133d cos(157.7deg + 0.0359deg*E).
CS    Lac    Min II 9.4.
CZ    Lac    Delta(S) = 1. P var. Max = 2432878.234 + 0.43210346d*E
             (JD2428700 - 39400) [01442]; Max = 2443081.309 +
             0.4319850d*E (JD2439400 - 43100) [05839]; Max =
             2444080.122 + 0.432114d*E (JD2443800 - 44100)
             [09009]; since JD2445100 - see Table.
DD    Lac    VB A (B 9.2m, 69", 16deg).  P var. Max = 2421914.178 +
             0.19309018d*E - 0.001798d*10**(-8)*E**2 (JD2421400 -
             37600) [05711]; since JD2443000 - see Table.
             According to [09337] simultaneously the pulsations with
             the following periods are observed (the corresponding AB
             values are given in the brackets): P1 = 0.193082d (0.080m),
             P2 = 0.197382d (0.034m), P3 = 0.182115d (0.020m),
             P4 = 0.187438d (0.016m), P5 = 0.095109d (0.010m),
             P6 = 0.23583d (0.008m). A var; 0.04m <= A <= 0.12m.
DE    Lac    Delta(S) = 5. P var. Max = 2428807.130 + 0.2536940d*E
             (JD2427000 - 33000); Max = 2433005.766 + 0.2536929d*E
             (JD2433000 - 39100) [03378]; since JD2442000 - see Table.
DF    Lac    [A/H] = 0.2.
DG    Lac    P var. Min = 2426266.355 + 2.206435d*E (JD2426200 - 40000)
             [04961]; since JD2440000 - see Table.
DH    Lac    P var. Max = 2418240 + 284.8d*E (JD2418000 - 27350);
             since JD2427300 - see Table.
DM    Lac    Erroneously labeled VV306, instead of VV307, in the chart [05862].
DO    Lac    According to [00085], EA.
EG    Lac    P > 50d? [05386].
EM    Lac    Min II 13.09.
EN    Lac    VB A (B 11.32mV, 27", 345deg; C 9.0mV, 62", 48deg); SB1
             (Porb = 12.0968d). Eclipsing system with a pulsating
             primary component of BCEP type. Depth of Min I 0.05mB.
             Min I = 2444909.4339 + 12.096816d*E; D = 0.015P,
             d = 0.000P. Simultaneously pulsations are
             observed with the periods P1 = 0.169170d, P2 = 0.170770d,
             P3 = 0.181692d [09346]. The corresponding amplitudes
             of pulsations vary. The values of the amplitudes in
             B system are as follows: A1 = 0.046m, A2 = 0.024m,
             A3 = 0.022m (1952 - 1965); A1 = 0.016m, A2 = 0.010m,
             A3 = 0.014m (1977); A1 = 0.010m, A2 = 0.014m, A3 = 0.023m
             (1980 - 81). 0.01m <= A <= 0.11m.
EO    Lac    Min II 12.9; Min II - Min I = 0.485P.
EP    Lac    Depth of Min II 0.04m.
ER    Lac    Depth of Min II 0.05m:.
ES    Lac    Min II 11.6; Min II - Min I = 0.57P.
             Apsidal motion is possible:
             Min II = 2433582.95 + 4.459451d*E [09347].
EU    Lac    The chart in [05862] is wrong.
EV    Lac    VB A (B 12.74mB, 10", 260deg, 1949); mu alpha = -0.065s,
             mu delta = -0.46". Dark companion (A = 0.0206", P = 45 yr,
             E = 0.5) [09348]. In 1979 sinusoidal light oscillations
             were observed in the range 10.20m - 10.27mV:
             Min = 2444037.576 + 4.378d*E [09349]. In 1974 - 76 such
             periodicity was not observed [09350].
EW    Lac    Non-radial pulsations with P = 0.7d - 0.8d
             are also possible [09351, 09352].
EX    Lac    d = 0.050P.
FQ    Lac    A var; P var. Elements given in the Table are valid in the
             intervale JD2427950 - 31700.
FU    Lac    d = 0.013P.
GS    Lac    Min II 15.2.
GX    Lac    Min II 10.23.
HK    Lac    SB1 (Porb = 24.4284d [09355]).
HM    Lac    Depth of Min II 0.05m.
HN    Lac    Min II 14.7.
HQ    Lac    Erroneously labeled VV307, instead of VV306, in the chart [05862].
HR    Lac    Min II 14.3.
HT    Lac    In the region of the open cluster NGC 7209.
HW    Lac    Min II 14.8.
HX    Lac    Min II 14.8.
HZ    Lac    Min II 15.0.
IM    Lac    Min II 13.2.
IN    Lac    E?
IP    Lac    Min II 14.0.
IR    Lac    Min II 15.4; d = 0.03P.
IT    Lac    P var.
IU    Lac    Min II 13.5.
IY    Lac    Blazhko effect?
IZ    Lac    Min II 12.7.
KO    Lac    Min II 14.7.
KP    Lac    P < 1d.
KR    Lac    Min II 15.8; dII = 0.05P.
KS    Lac    Depth of Min II 0.03m.
KU    Lac    Depth of Min II 0.03m.
LU    Lac    Min II 15.32.
LW    Lac    d = 0.03P. Depth of Min II 0.03m?
LY    Lac    Min II 12.6.
LZ    Lac    Min II 12.5.
MO    Lac    d = 0.04P. Depth of Min II 0.05m.
MP    Lac    Min II 12.5.
MV    Lac    Min II 15.0.
MZ    Lac    Min II 12.1; Min II - Min I = 0.713P.
             Min II = 2433872.702 + 3.158719d*E. Elements for Min I
             are given in the Table.
NN    Lac    d = 0.02P. np (usually brighter) component of a close pair.
             The range of combined brightness is given in the Table.
NO    Lac    Depth of Min II 0.03m.
NR    Lac    Min II 13.4. Sp (brighter) component of a close pair. The
             range of combined brightness is given in the Table.
NU    Lac    EW?
NW    Lac    Min II 13.9. Close binary, the components of which are
             equal in brightness at minimum light. The range of
             combined brightness is given in the Table.
OO    Lac    Min II 12.8.
OV    Lac    150d <= P <= 200d.
OX    Lac    Depth of Min II 0.04m.
PP    Lac    Min II 12.0.
PT    Lac    Min II 15.4.
PZ    Lac    In the region of the open cluster NGC 7243.
QQ    Lac    In the region of the open cluster NGC 7243.
QU    Lac    Depth of Min II 0.04m.
V0335 Lac    Min II 15.8.
V0338 Lac    In the region of the open cluster IC 1434.
V0339 Lac    P = 3.4084964d?
V0340 Lac    Min II 12.4; Min II - Min I = 0.762P;
             Min II = 2432858.521 + 19.943102d*E.
             Elements for Min I are given in the Table.
V0342 Lac    Min II 12.9.
V0343 Lac    Min II - Min I = 0.57P. Depth of Min II 0.03m:.
V0344 Lac    Min II 13.0. Min I = 2433873.5784 + 0.39222768d*E
             (JD2432800 - 35800); since JD2445200 - see Table.
V0345 Lac    Min II 11.6; Min II - Min I = 0.340P; DII = 0.040P;
             dII = 0.014P. Apsidal motion is possible.
V0347 Lac    VB.
V0350 Lac    VB A (B 9.7m, 66", 94deg); SB1 (P = 17.755d [09356]).
             Min II 6.45 [07468]. Mean magnitude varies. See also [08933].
V0355 Lac    Northern component of a pair.
V0360 Lac    SB2 (P = 10d [09357]). Min II 5.93.
V0362 Lac    VB A (B 13.2m, 1.8", 49deg).
V0363 Lac    VB A (B 11.3m, F6 III - V:, 6.3", 325deg).
V0364 Lac    Min II 9.15; Min II - Min I = 0.52P; dI = 0.003P,
             DII = 0.077P, dII = 0.009P.
V0412 Lac    SB, Porb = 41.95yr.
V0413 Lac    SB, Porb = 2.9833d.
V0442 Lac    Quasi-periodic brightness variations of a planetary nebula, possibly
             due to variable mass loss or pulsations.
R     Leo    P var. Max = 2385112 + 312.43d*E (JD2385100 - 2402500);
             Max = 2402929 + 314.33d*E (JD2402500 - 11500);
             Max = 2411416 + 308.93d*E (JD2411500 - 16500);
             Max = 2416984 + 317.84d*E (JD2416500 - 22500);
             Max = 2423328 + 312.75d*E (JD2422500 - 27000);
             Max = 2427081 + 307.40d*E (JD2427000 - 30000);
             Max = 2437337 + 312.13d*E (JD2430000 - 37500);
             since JD2437500 - see Table. SiO, H2O, OH maser.
S     Leo    P var. Max = 2420654 + 189.24d*E (JD2420200 - 26100);
             Max = 2426142 + 185.92d*E (JD2426100 - 28100);
             since JD2428100 - see Table.
T     Leo    SB1 (Porb = 0.05881873d [09304]).
V     Leo    H2O maser.
W     Leo    P var. Max = 2434651 + 385.41d*E (JD2409500 - 35000);
             since JD2437500 - see Table. OH maser.
Y     Leo    P var. Min = 2422372.520 + 1.6860978d*E (JD2418000 - 23500)
             [02389]; Min = 2422372.5368 + 1.68607314d*E
             (JD2423500 - 38600) [09307]; since JD2438600 - see Table.
             There is periodic term in the elements given in the Table:
             +0.00375d*sin(0.21487deg*E + 141.7deg). Depth of Min II
             0.1m IR.
RR    Leo    Delta(S) = 7.1. P var. Max = 2430440.3385 + 0.45238172d*E +
             1.963d*10**(-10)*E**2 (1898 - 1977) [08299]; since
             JD2441400 - see Table.
RT    Leo    Min II 10.5.
RW    Leo    P var. Before JD2440800 Min = 2424993.458 +
             1.6825365d*E [03115]; since JD2440800 - see Table.
RX    Leo    Delta(S) = 6.8.
SS    Leo    P var. Max = 2415485.723 + 0.62633242d*E
             (JD2414000 - 22000) [00752]; since JD2422000 - see Table.
             [Fe/H] = -1.59.
ST    Leo    (k - b)2 = 0.08.
SZ    Leo    P var. Before JD2442500 Max = 2425331.400 +
             0.5340833d*E [04157]; since JD2442500 - see Table.
             Light curve shape var?
TV    Leo    P var. Max = 2419852.318 + 0.6728362d*E
             (JD2419000 - 28000) [00001]; since JD2437000 - see Table.
             (k - b)2 = -0.01.
TX    Leo    VB A (B 7.8m, 2", 157deg, 1971);
             A binary according to lunar occultation data: ro = 0.0005".
             The range of combined brightness is given.
             Min II 5.69; DII = 0.19P; Min II - Min I = 0.550P.
TY    Leo    Elements need confirmation.
TU    Leo    Minor planet (8) Flora.
UU    Leo    Min II 11.5. P var. Since JD2430000 - see Table.
UV    Leo    Min II 9.49; d = 0P014. P var. Before JD2434000
             Min I = 2425574.302 + 0.60008516d*E [07554];
             since JD2434000 - see Table.
UX    Leo    Min II 10.4.
             Moments of Min by BBSAG contradict the tabulated elements.
UZ    Leo    Min II 10.12. P var, nonlinear term: +2.8d*10**(-12)*E**2.
XX    Leo    Min II 11.4. Period should be checked.
XY    Leo    Min II 9.80. P var. Min = 2435195.66306 + 0.2841091d*E
             (JD2434000 - 36500) [03392]; Min = 2437376.465 +
             0.28409592d*E (JD2436500 - 40000) [00001]; Min =
             2441005.5364 + 0.28410727d*E (JD2441000 - 44000)
             [09084]; since JD2444000 - see Table.
             The light curve shape var.
XZ    Leo    Min II 11.1.
AB    Leo    Epoch of Min is given.
             According to [01853], Max = 2428880 +
             103.2d*E (JD2414600 - 19000, 2428000 - 31600);
             During other time intervals cycles 75d - 125d.
AD    Leo    mu = 0.49", P = 265deg; pi = 0.20".
             X-ray and radio source. Astrometric binary?
AF    Leo    H2O maser.
AM    Leo    VB A (B 10.64m, 11", 270deg). Min II 9.83.
AP    Leo    Min II 9.88. P var. Min = 2414986.868 + 0.430350d*E
             (JD2414700 - 18600); since JD2418600 - see Table.
             Light curve shape var.
AQ    Leo    Elements for fundamental mode pulsations (P0) see Table.
             For the first overtone: P1 var?;
             P1 = 0.4101369d (1929 - 1969); P1 = 0.410130d (1957 -
             1969); during 1973 - 1975 Max1 =
             2441766.486 + 0.4101487d*E. delta(M0) = 0.23m,
             delta(M1) = 0.46M.
AU    Leo    Vr = +7545 km/s. Variability is doubtful.
BB    Leo    [Fe/H] = -1.32.
BL    Leo    Min II14.4. P var. Since JD2442000 - see Table.
BV    Leo    Min II 16.1.
BW    Leo    Min II 15.4.
BX    Leo    [Fe/H] = -1.23.
BZ    Leo    Min II 15.8.
CD    Leo    Light curve shape var.
CE    Leo    Min II 12.5. P var?
             Min by BBSAG contradict the tabulated elements.
CN    Leo    Mu = 4.7", P = 235deg; pi = 0.41".
             Soft X-ray source, radio source.
CW    Leo    Dust envelope, 6"*4".
             Molecular radioemission: SiO, SiS, HCN, HC3N, CO, H2O,
             NH3, etc. Polarization in I band up to 24%.
CX    Leo    VB A (B 12.3m, 132deg); SB (Porb = 12685.4d).
CY    Leo    mu = 0.307", P = 141.3deg; pi = 0.022".
             Outside flares Delta(m) < = 0.036m; P = 600s, 822s, 1638s
             [06209]. A single strong flare with delta(M) = 0.61m in
             blue light of 10 Min duration was observed [06141],
             which is attributed by several authors to the presence of
             a red flaring companion.
DE    Leo    P = 1.2d - 2.0d?
DG    Leo    VB B (A 6.6m, A 8IV, SB2, Porb = 4.15d; B 6.9m, 0.271",
             211.2deg, 1980, Porb ~200yr).
             The range of the bombined brightness is given.
DH    Leo    SB1, Porb = 1.070354d.
DK    Leo    mu alpha = -0.097", mu delta = -0.214".
FL    Leo    Variability range according to E.M. Halbedel, IBVS No. 3502, 1990.
FX    Leo    Not a nearby star (despite having a Gl number).
R     LMi    SiO, H2O, OH mazer.
T     LMi    Min II 10.97. P var. Min I = 2420573.698 + 3.019889d*E
             (JD2420200 - 25000); Min I = 2423856.323 +
             3.0199336d*E (JD2423800 - 35500); since JD2438400 - see
             Table.
U     LMi    1m <= A <= 3.3m. Periodicity sometimes breaks down.
V     LMi    Delta(S) = 5.7.
Y     LMi    P var. Max = 2428636.322 + 0.52443938d*E + 0.0597d*
             *sin(0.0657deg*E + 27.2deg) (JD2425250 - 28500); Max =
             2428636.348 + 0.5244564d*E (JD2428500 - 30000)
             [01856]; mean elements
             for interval JD2432200 - 38900 are given in the
             Table; in this interval the period changed with the
             cycle of ~2100d. Blazhko effect with the period 33.4d
             [01856]; 07m <= A <= 1.9m, 0.19P <= m - M <= 0.44P.
RT    LMi    Min II 11.7.
RU    LMi    Spectrum description [09326].
RW    LMi    VB A (B 15.5m B, 9", 10deg). 0.3m - 2.6m K, 7.64m - 10.71m,
             9.7m - 14.6m R, 14.1m - 18.1m B, 14.8m - 18.6m U.
             Mean brightness varies. Gaseous-dust circumstellar
             envelope. CO emission. Spectrum description [09327].
RY    LMi    VB A (B 16.1m, dM2, 15", 126deg); mu = 0.14", P = 264deg.
             P0 = 215.197388s, dP0/dt = 5.6s*10**(-14)/s, A0 = 0.0440m;
             P1 = 304.4s, A1 = 0.0150m; P2 = 271.0s, A2 = 0.0134m;
             P3 = 107.6s, A3 = 0.0032m; P4 = 126.2s, A4 = 0.0028m;
             P5 = 119.8s, A5 = 0.0026m.
             Mean brightness varies by 0.05m.
R     Lep    P var. Max = 2398883 + 436.44d*E (JD2398000 - 2412000);
             Max = 2412849 + 418.04d*E (JD2412000 - 23000);
             Max = 2423300 + 441.38d*E (JD2423000 - 36000);
             since JD2436000 - see Table.
             A var; 5.5m <= Max <= 9.5m (Possible period is more
             than 40 years [03402]).
S     Lep    Mean magnitude varies with the cycle of 890d. H2O maser.
T     Lep    SiO maser.
U     Lep    P var. Max = 2425084.431 + 0.58147098d*E
             (JD2411000 - 25090); Max = 2425084.431 + 0.58147377d*E
             (JD2425080 - 37700) [03403]; since JD2436600 - see Table.
             Delta(S) = 8.5; (k - b)2 = 0.00.
V     Lep    Min II 9.9.
Z     Lep    Min II 12.0:.
RR    Lep    Min II 10.4.
RS    Lep    Min II 9.96.
RU    Lep    P var?
RZ    Lep    S 4/4.
SS    Lep    SB2 (Porb = 258.2d [09363]).
SY    Lep    VB A (B 15.2m: V, 18", 270deg).
S     Lib    P var. Max = 2405692 + 192.14d*E (JD2402700 - 24000);
             Max = 2424141 + 194.74d*E (JD2424000 - 30500);
             Max = 2431900 + 190.34d*E (JD2430500 - 37200);
             Max = 2439203 + 197.61d*E (JD2437200 - 39300);
             since JD2441000 - see Table. Mean value of the period is
             given in the Table. A var (1.8m <= A <= 5m).
W     Lib    P var. Max = 2412272 + 203.76d*E (JD2412000 - 28500);
             Max = 2428573 + 201.48d*E (JD2428500 - 34000);
             since JD2434000 - see Table.
X     Lib    P var. Max = 2423500 + 165.75d*E (JD2413000 - 25000);
             since JD2425000 - see Table.
Y     Lib    P var. Max = 2413452 + 275.7d*E (JD2413400 - 22000);
             Max = 2422273 + 272.5d*E (JD2422000 - 28000) [00458];
             Max = 2434921 + 277.04d*E (JD2428000 - 35000);
             since JD2435000 - see Table.
Z     Lib    P var. Max = 2417736 + 294.5d*E (JD2407100 - 17800);
             since JD2424400 - see Table.
RR    Lib    P var. Max = 2409699 + 277.4d*E (JD2409600 - 15600);
             Max = 2416345 + 273.2d*E (JD2416300 - 19700);
             Max = 2421027 + 278.6d*E (JD2421000 - 27150) [00458];
             since JD2427150 - see Table.
RS    Lib    P var. Max = 2413396 + 217.2d*E (JD2413300 - 20000);
             Max = 2420110 + 219.6d*E (JD2420000 - 27500) [00458];
             Max = 2429078 + 215.6d*E (JD2427500 - 35000);
             Max = 2438196 + 219.9d*E (JD2435000 - 42600);
             since JD2441700 - see Table.
RT    Lib    P var. Max = 2413776 + 254.21d*E (JD2413000 - 19000);
             since JD2419000 - see Table.
RU    Lib    P var. Max = 2413363 + 312.0d*E (JD2413300 - 16200);
             Max = 2416807 + 322.5d*E (JD2416800 - 21000);
             Max = 2421309 + 317.0d*E (JD2421300 - 24200);
             Max = 2424804 + 311.5d*E (JD2424800 - 29800) [00458];
             Max = 2434909 + 319.9d*E (JD2429800 - 35000); since
             JD2437700 - see Table.
RV    Lib    Min II 9.44.
RX    Lib    [A/H] =  -0.5. P var. Max = 2430913.6 + 24.950d*E
             (JD2425000 - 36300) [00266]; since JD2436300 - see Table.
SS    Lib    Min II 10.8; d = 0.030P.
ST    Lib    VB A (B 14m, 14", 0deg).
TV    Lib    Delta(S) = 2.5.
TY    Lib    d = 0.019P.
UW    Lib    [Fe/H] =  - 0.25.
VV    Lib    P var. Max = 2424268.474 + 0.4781418d*E
             (JD2419800 - 2425000); since JD2425000 - see Table.
VW    Lib    Observations given in
             [00293] contradict the elements given in the Table.
VY    Lib    P var? [03506].Delta(S) = 6.
VZ    Lib    Min II 10.55; dI = 0.000P; dII = 0.005P. P var. Min I =
             2429022.227 + 0.358053d*E (JD2428600 - 30400)
             [09368]; Min I = 2430899.223 + 0.358448d*E
             (JD2430400 - 32400) [02532]; since JD2444330 - see Table.
YZ    Lib    Min II 12.9.
AA    Lib    P var? The elements are valid in the interval
             JD2427800 - 29600.
AF    Lib    The chart in [06286] has south on top.
AP    Lib    Z = 0.0486.
AQ    Lib    [Fe/H] = -0.60.
BE    Lib    The chart in [06286] is wrong.
BH    Lib    Recommended chart in [06286]: part III, page 50.
BT    Lib    Min II 12.3.
BW    Lib    The chart in [06286] is wrong.
CG    Lib    [Fe/H] = -1.82. P var. Max = 2438592.287 + 0.3068674d*E
             (JD2427800 - 39600) [07557]; since JD2439600 - see Table.
CQ    Lib    The coordinates in [01870] are wrong.
CZ    Lib    The chart in [06286], part I, page 40 is wrong. Recomended
             chart in [06286]: part III, page 52.
EH    Lib    Delta(S) = 0. 9.35m <= Max < = 9.49m V;
             Max (A) = 2442162.556 + 0.273778d*E [09336].
ES    Lib    Min II 7.33.
EU    Lib    70d <= P <= 90d.
FI    Lib    90d <= P <= 110d.
FS    Lib    OH emission.
FX    Lib    Spectrum description  [06167, 09371].
del   Lib    VB A (B 11.3m, 9", 351deg; C 12.80m, 67", 90deg); Min II
             4.98. P var?
S     Lup    VB A (B = X Lup, 13", 176deg). P var. Max = 2411950 +
             347.81d*E (JD2411950 - 14000); Max = 2414040 +
             339.31d*E (JD2414000 - 19000); Max = 2419135 +
             345.12d*E (JD2419000 - 26000); Max = 2426038 +
             336.60d*E (JD2426000 - 29500); Max = 2429743 +
             345.15d*E (JD2429500 - 35000); since JD2437600 - see Table.
X     Lup    VB B (A = S Lup).
Y     Lup    P var. Max = 2424691 + 408.15d*E (JD2423000 -
             25500); Max = 2425503 + 394.81d*E (JD2425500 -
             30250); Max = 2430641 + 407.75d*E (JD2430250 -
             35000); since JD2437900 - see Table.
RU    Lup    Sometimes varies quasiperiodically: P1 = 3.5457d, P2 =
             3.8375 [02412]. H2O maser.
RY    Lup    Quasiperiodicity: P = 3.7609d [09366].
SX    Lup    Min II 11.8.
TY    Lup    The chart in [06286] is wrong.
UX    Lup    [A/H] = -0.9. P var. P = 16.2403d (JD2411526 -
             14040); P = 16.2065d (JD2414040 - 24016); P =
             16.2492d (JD2424016 - 25638); P = 16.1794d
             (JD2425638 - 26449); P = 16.2241d (JD2426449 - 29693)
             [05387].
VV    Lup    Close northern companion.
VZ    Lup    P var? Light curve shape var?
CC    Lup    The chart in [06286] is wrong.
CW    Lup    The charts in [06286] are wrong.
CX    Lup    Min II 12.8.
CY    Lup    High Max every 360d, especially faint Min 80d before
             these high Max.
DG    Lup    Min II 15.1.
DQ    Lup    The chart in [06286] is wrong.
DY    Lup    In [00087] the information on variability of DY Lup is
             accompanied by the coordinates of DZ Lup and vice versa.
             The chart for DY Lup in [06286] is labeled DZ Lup, the
             chart for DZ Lup in [06286] is wrong.
DZ    Lup    In [00087] the information on variability of DY Lup is
             accompanied by the coordinates of DZ Lup and vice versa.
             The chart for DY Lup in [06286] is labeled DZ Lup, the
             chart for DZ Lup in [06286] is wrong.
EL    Lup    VB.
ER    Lup    P2 = 140d.
EU    Lup    The chart in [06286] is wrong.
FK    Lup    Min II 10.7:.
FM    Lup    The chart in [02385] is wrong.
FR    Lup    Deep Min II.
FT    Lup    Min II 9.98. dI = 0.025P?, dII >= 0.066P. P var.
             Before JD2439300 Min I = 2427987.310 + 0.470089d*E
             [03948]; since JD2445000 - see Table. All the observations
             are well represented also by the elements:
             Min I = 2445061.834 + 0.470083d*E - 0.114d*10**(-9)*E**2
             [09360]. Light curve shape var?
FV    Lup    Min II 11.2.
GG    Lup    Min II 5.8.
GN    Lup    VB A (B 10.2m vis, 10", 98deg).
GO    Lup    Relatively short P.
GW    Lup    In the dark nebula Barnard 228.
HK    Lup    B - V: +1.23, +1.46.
HL    Lup    The initial identification with 2U 1543 - 47 is wrong.
             2U 1543 - 47 = IL Lup.
HM    Lup    B - V: +1.12.
HN    Lup    B - V: +1.55, +1.68.
HO    Lup    B - V: +0.70, +0.81.
alf   Lup    VB A (B 14.0m, 27.6", 232deg, 1901).
             Soft X-ray source. P2 = 3.145d is possible [08417].
gam   Lup    SB, Porb = 2.8081d.
del   Lup    Less probable variant of elements:
             Max = 2441045.160 + 0.14273*E.
R     Lyn    S 4/5E - S 6/6 - .
S     Lyn    VB A (B 14m, 12.6", 155deg). P var. Max = 2414564 +
             300.26d*E (JD2414500 - 27400); Max = 2434241 +
             294.42d*E (JD2427400 - 35100); Max = 2440225 +
             300.44d*E (JD2435100 - 40220); since
             JD2440220 - see Table.
T     Lyn    P var. Max = 2425012 + 419.0d*E (JD2412800 - 34700);
             since JD2434700 - see Table.
U     Lyn    H2O, OH emission. P var. Max = 2417168 +
             440.3d*E (JD2417100 - 26000) [00458]; Max =
             2435908 + 432.05d*E (JD2426000 - 36000); Max =
             2439898 + 447.1d*E (JD2436000 - 40000); since
             JD2440000 - see Table.
V     Lyn    Cycles 55d and 87d replace one another. Mean brightness
             varies.
Y     Lyn    SB.
RR    Lyn    VB A (B 10m, 50"). Min II 5.90; Min II = 2438051.3115 +
             9.945074d*E; E = 0.081; Min II - Min I = 0.45P (JD2437700).
RW    Lyn    [Fe/H] = -1.37.
RZ    Lyn    Min II 10.8.
SW    Lyn    Min II 9.65; dI = 0.038P. P var. Min I = 2425643.323 +
             0.6440661d*E (JD2425640 - 35850) [02742]; Min I =
             2438795.8016 + 0.6440520d*E (JD2438380 - 840)
             [09387]; Min I = 2440614.0107 + 0.6440729d*E
             (JD2439500 - 40620) [00001]; Min I = 2442786.4493 +
             0.6440677d*E (JD2440650 - 42790) [07292];
             since JD2442780 - see Table.
SX    Lyn    Min II 10.1. P var. Min I = 2428636.375 + 2.0225615d*E
             (JD2427400 - 34700) [00519]; Min I = 2442561.424 +
             2.0225172d*E (JD2442400 - 44000); since JD2444000 - see
             Table.
SZ    Lyn    SB (Porb = 1146d, E = 0.26 [09388]). Delta(S) = 0.
             There is a periodical term in the elements:
             -0.00573d cos 2pi (EP0/P1 + 0.007); P0 = 0.120534920d,
             P1 = 1150d. Amplitude and shape of the light curve vary.
TT    Lyn    Delta(S) = 7.
TV    Lyn    [Fe/H] = -0.99.
TW    Lyn    Delta(S) = 10. P var. Max = 2418676.804 + 0.4817201d*E
             (JD2418670 - 20155); Max = 2420155.685 + 0.4816929d*E
             (JD2420155 - 27480); Max = 2427479.359 + 0.4817481d*E
             (JD2427480 - 28630);
             Max = 2428627.310 + 0.4818529d*E (JD2428620 - 37800)
             [02819]. Since JD2445000 - see Table.
TZ    Lyn    Epoch of Min brightness is given.
UU    Lyn    Min II 11.82.
UV    Lyn    Min II 9.78.
UZ    Lyn    VR var (P = 0.065d [09392]).
VV    Lyn    VB A (B 11.76m, 38.6",354deg); SB; mu alpha = -0.0285S,
             mu delta = -0.274".
VW    Lyn    P1 = 590s, P2 = 260s [09393].
CW    Lyn    Type RRC: is also possible.
S     Lyr    P var. Max = 2416186 + 432.01d*E (JD2415700 - 20100);
             Max = 2420961 + 445.83d*E (JD2420900 - 26500);
             Max = 2426748 + 429.01d*E (JD2426500 - 30700);
             Max = 2432357 + 441.88d*E (JD2432000 - 34600);
             since JD2442500 - see Table.
U     Lyr    VB A (B 13.0m, 9.4", 182deg). P var. Max = 2418345 +
             459.22d*E (JD2418000 - 27000); since JD2432000 - see
             Table.
V     Lyr    OH maser.
W     Lyr    P var. Max = 2415578 + 198.39d*E (JD2413000 - 19000);
             Max = 2420322 + 194.99d*E (JD2419000 - 25500);
             Max = 2431326 + 198.97d*E (JD2427000 - 31500);
             Max = 2432494 + 195.11d*E (JD2431500 - 36500);
             since JD2437500 - see Table.
Y     Lyr    Delta(S) = 0.8.
Z     Lyr    P var. Max = 2418150 + 285.07d*E (JD2417500 - 22200);
             Max = 2423600 + 291.37d*E (JD2422200 - 29500);
             Max = 2430000 + 284.00d*E (JD2429500 - 36800);
             since JD2436800 - see Table.
RR    Lyr    mu alpha = -0.11", mu delta = -0.19". [Fe/H] = -1.14;
             Delta(S) = 6. Blazhko effect of variable
             amplitude (practically to complete disappearance of
             Blazhko effect); Pi = 40.8d. Variations of Max light
             phase up to 0.14P; magnitude in Max var in the range
             up to 0.6m, that in Min var in the range up to 0.1m
             [03418].According to [07270], a cycle ~4 yr is present
             in Blazhko effect amplitude changes; at the end of
             the cycle the Blazhko effect phase changes abruptly
             by 0.25Pi. Magnetic field strength varies with the
             pulsational period [09339].
             P var. Max = 2414856.480 + 0.56682069d*E
             (JD2414800 - 18800); Max = 2421854.052 + 0.56685169d*E
             (JD2418800 - 26500) [09379]; Max = 2426571.3828 +
             0.56684333d*E (JD2426500 - 32500) [09338]; Max =
             2438215.9492 + 0.566830d*E (JD2438000 - 41000)
             [05238]; Max = 2438215.9492 + 0.56683313d*E
             (JD2441000 - 42900) [09338]; since JD2442900 - see Table.
RS    Lyr    P var. Max = 2415566 + 299.38d*E (JD2415000 - 24000);
             Max = 2425176 + 308.08d*E (JD2424000 - 37200);
             since JD2437200 - see Table.
RT    Lyr    P var. Max = 2437022 + 250.85d*E (JD2415000 - 39000);
             since JD2439000 - see Table.
RU    Lyr    P var. Max = 2415983 + 370.70d*E (JD2415900 - 33000);
             Max = 2433035 + 363.0d*E (JD2433000 - 41000);
             since JD2441000 - see Table.
RV    Lyr    D = 0.015P. P var. Min = 2415949.7096 + 3.599007d*E
             (JD2412185 - 16000); Min = 2415949.7096 +
             3.599046d*E (JD2416000 - 21400) [00001];
             Min = 2432015.671 + 3.5989845d*E (JD2421400 - 32000);
             Min = 2432015.671 + 3.5990235d*E (JD2432000 -
             39300) [09085]; since JD2442000 - see Table.
RW    Lyr    OH, H2O maser.
RX    Lyr    P var. Max = 2416226 + 249.94d*E (JD2415000 - 28800);
             since JD2428800 - see Table.
RZ    Lyr    P var. Max = 2416415.360 + 0.51127069d*E
             (JD2413000 - 19000) [00001]; Max = 2426161.4375 +
             0.51124948D*E (JD2426000 - 38000) [00323];
             since JD2438000 - see Table.
             Blazhko effect, height of Max varies: 10.6m - 10.9m,
             Max (Delta(m)) = 2430904.3 + 116.654d*N + 0.01034d*N**2;
             Min (Delta(m)) - Max (Delta(m)) = 59.3d [03419].
             [Fe/H] = -1.69; Delta(S) = 10.0.
SS    Lyr    P var. Max = 2421695 + 350.48d*E (JD2416000 - 22500);
             Max = 2429991 + 355.22d*E (JD2429000 - 38000); since
             JD2438000 - see Table.
SZ    Lyr    According to [05750], during JD2434665 - 35044 the
             amplitude was twice smaller than usual (due to the depth
             of Min), and a temporary phase shift by 0.5P occured.
TT    Lyr    d = 0.010P; Min II 9.44.
TW    Lyr    VB A (B 15.2m pg, 14".70deg, 1912).
TY    Lyr    P var. Max = 2419285 + 336.49d:*E (JD2419000 - 23700);
             Max = 2423985 + 329.79d*E (JD2423700 - 31250);
             since JD2438600 - see Table.
TZ    Lyr    VB A (B 12.29m, 2.54", 2.5deg). Min II 11.05. P var.
             Min I = 2420669.480 + 0.5288234d*E (JD2420000 - 38000);
             since JD2438000 - see Table.
UX    Lyr    B - V: +0.11, +0.47.
UZ    Lyr    d = 0.012P:. P var. Min = 2424268.474 + 1.891253d*E
             (JD2422500 - 25500) [02087]; since JD2425500 - see Table.
AA    Lyr    Min II 13.5.
AH    Lyr    d = 0.03P. Min II 12.1.
AK    Lyr    Min II 12.9.
AL    Lyr    P var. Max = 2427865.82 + 12.9837d*E (JD2414800 - 28000)
             [00001]; Max = 2432889.03 + 12.98047d*E
             (JD2428000 - 35500) [04427]; since JD2435500 - see Table.
AQ    Lyr    P var. Max = 2425301.592 + 0.3571721d*E
             (JD2425300 - 29000); Max = 2428944.739 + 0.3571285d*E
             (JD2429000 - 30200); Max = 2430158.976 + 0.3571611d*E
             (JD2430200 - 33900); Max = 2433909.178 + 0.3571861d*E
             (JD2433900 - 35700); during JD2435700 - 37800 - see Table.
             Blazhko effect? According to visual observations,
             0.4m <= Delta(m) <= 1.2m.
AY    Lyr    Cycles of supermaxima 188.9d - 212.8d.
             Superhumps period: Ps = 0.07552d [06249].
BF    Lyr    P var. Max = 2425296 + 130d*E (JD2425300 - 800);
             During JD2429045 - 570 - see Table.
BH    Lyr    P var. Max = 2413712.358 + 0.6129028d*E
             (JD2413712 - 27927); Max = 2434472.547 + 0.6128941d*E
             (JD2434472 - 36102); since JD2436423 - see Table.
BQ    Lyr    Delta(S) = 0:.
BV    Lyr    d = 0.025P.
CC    Lyr    P var. Max = 2433182.7 + 24.028d*E (JD2426100 - 33400);
             Max = 2437078.8 + 24.200d*E (JD2433400 - 37100) [00001];
             Max = 2439418.5 + 24.185d*E (JD2437100 - 39420) [05644];
             since JD2440400 - see Table. Light curve shape var?
             [A/H] = -2.2.
CV    Lyr    Possible superposition of P2 = 135d.
CX    Lyr    P var. Max = 2418596.111 + 0.616689d*E
             (JD2414880 - 20000); Max = 2427696.396 + 0.616669d*E
             (JD2427530 - 30610); since JD2433000 - see Table.
             Delta(S) = 7:.
DD    Lyr    P var. Max = 2425494.334 + 0.372610d*E (JD2418900 - 27600)
             [00001]; since JD2427600 - see Table.
DF    Lyr    Min II 13.4.
DI    Lyr    P var. Max = 2437160.310 + 0.4174486d*E (JD2437160 - 39293);
             Max = 2439293.468 + 0.4178451d*E (JD2439293 - 40768);
             since JD2440768 - see Table.
DN    Lyr    P2 = 600d.
DR    Lyr    [Fe/H] =  -1.41; Delta(S) =7.4.
DU    Lyr    Min II 13.3.
EN    Lyr    B - V: + 0.40. + 0.43. P var. Delta(m) var.
EP    Lyr    Max I ” = 0.20P; Min II 10.36m - 10.58m,  ” = 0.50P;
             Max II 10.01m - 10.10m,  ” = 0.70P.
             Secondary oscillations: P2 = 45.1d,  P3 = 7067d [09354].
EW    Lyr    P var; nonlinear term:
             +0.00210d*10**(-6)*E**2 (JD2426500 - 45500);
             since JD2442000 the observations are represented also by
             the elements: Min = 2445597.391 + 1.948763d*E [07037, 00001].
EX    Lyr    [Fe/H] = -0.63; Delta(S) = 2.5.
EZ    Lyr    VB A (B 12.3m, 14", 302deg, 1934). P var. Since
             JD2426577 - see Table. Delta(S) = 7.1.
FG    Lyr    VB A (B 14m, <10"). d = 0.035P. P var?
FH    Lyr    P var?
FK    Lyr    The identification with HDE 337663(G5) [00021] is wrong.
FL    Lyr    Min II 9.52,  DII = 0.05P.
FN    Lyr    B - V: +0.15, +0.48.
FO    Lyr    Min II 13.7.
GY    Lyr    The elements describe the brightest maxima. Between them
             there are 2 - 3 waves of smaller amplitude. Red.
HP    Lyr    Min II 11.0.
HQ    Lyr    P var, periodic term: +30d*sin(8deg*E).
HT    Lyr    Min II 13.3.
HY    Lyr    Min II 14.1.
IK    Lyr    Blazhko effect?
IL    Lyr    According to [00569], Max = 2429375.519 + 0.377620d*E,
             M - m = 0.14P:.
IO    Lyr    Delta(S) = 3.
IP    Lyr    Min II 13.3.
IW    Lyr    Min II 13.3.
IY    Lyr    Min II 14.1.
KM    Lyr    Blazhko effect: Pi = 30d, 0.14P <= M - m <= 0.20P.
KP    Lyr    ADS 11423 C (A 8.5m, B 9.7m; AB - C 77", 208deg; D 13.1m,
             C - D 14", 61deg, 1904). P2 = 1300d is possible.
KR    Lyr    P var. The light curve shape var.
KT    Lyr    Min II 14.9.
KX    Lyr    Delta(S) = 0.
LQ    Lyr    [Fe/H] =  -1.39; Delta(S) = 7.2.
LR    Lyr    P var? [Fe/H] = -1.41; Delta(S) = 7.4.
LT    Lyr    Rapid variation (0.5m in an hour) were observed.
LX    Lyr    Delta(S) = 8:.
LZ    Lyr    P var. Min = 2425347.565 + 1.611143d*E (JD2425347 - 32119)
             [00569]; since JD2442870 - see Table.
MN    Lyr    Min II 14.1.
MR    Lyr    Alternative P = 0.66d:.
MS    Lyr    P < 0.5d?
MT    Lyr    Min II 16.2.
MV    Lyr    SB (Porb = 0.1336d [09373]).
             Quasiperiodic fadings of different amplitude:
             Min = 2425558 + 455.5d*E (JD2425500 - 30100);
             Min = 2430113 + 325.3d*E (JD2430100 - 36900);
             Min = 2436944 + 357.8d*E (JD2436900 - 44100) [09372].
             After JD2444100 the mean brightness
             level became fainter by 5m; outbursts with an amplitude
             up to 3m of 1 - 2 months duration are observed [09404].
             During the bright level of light, flickering up
             to 0.4m in 5 Min in U bAnd is observed [00365]. Soft
             X-ray source.
             B - V: 0.00 +- 0.40; U - B:  -0.86 +  -1.30.
MW    Lyr    P var. Max = 2429521.386 + 0.3978817d*E (JD2427700 - 36000);
             since JD2436000 - see Table.
             Blazhko effect: Pi = 33.3d; the amplitude varies by 0.6m.
MZ    Lyr    Min II 14.0.
NV    Lyr    d = 0.02P:.
NW    Lyr    P var. Max = 2436483.323 + 1.6012330d*E (JD2414500 -
             36400) [03506]; since JD2436400 - see Table.
             B - V: +0.38, +0.86.
NY    Lyr    Min II 13.1.
NZ    Lyr    O - C vary harmonically with an amplitude +- 0.01d,
             Pi ~2500P.
OQ    Lyr    VB (B 12.1m vis, 5.3", 175deg, 1930).
OS    Lyr    40d <= P <= 60d. P2 = 400d - 500d is superimposed.
PQ    Lyr    d = 0.014P; Min II 14.9.
PS    Lyr    d = 0.02P:; Min II 11.4.
PU    Lyr    Close companions sf, s.
PV    Lyr    d = 0.03P:.
PY    Lyr    Min II 13.4. P var. Min I = 2434980.4372 + 0.38576671d*E
             (JD2432700 - 36900) [04248]; since JD2442500 - see Table.
QQ    Lyr    Min II 14.6.
QT    Lyr    Min II 14.6.
QU    Lyr    Min II 13.1.
V0335 Lyr    Large scatter in the light curve.
V0336 Lyr    P var. Min = 2429965.283 + 1.9049105d*E (JD2429370 - 31590);
             during JD2438930 - 40010 - see Table.
V0337 Lyr    Large scatter in the light curve.
V0348 Lyr    Min II 16.8.
             The elements are valid during JD2444023 - 45232.
V0350 Lyr    P var. The elements are valid during JD2438280 - 45232.
V0355 Lyr    The elements are valid during JD2429322 - 45232.
V0356 Lyr    VB A (B 17.5m, 10", 120deg, [00001]).
V0361 Lyr    Min II 15.3, Max II 14.7, Max II - Min I = 0.70P.
             The elements are valid during JD2433776 - 45232).
V0374 Lyr    Faint companions np, sf.
V0380 Lyr    Faint close companion nf.
V0385 Lyr    Faint close companion sf.
V0388 Lyr    No brightenings were observed during JD2438322 - 39289.
V0389 Lyr    The elements are valid during JD2438322 - 40007.
V0390 Lyr    The elements are valid during JD2439913 - 40007.
V0401 Lyr    Min II 14.4:. The period may be spurious.
V0403 Lyr    P var?, Pi = 500 P?
V0404 Lyr    Min II 12.4.
V0406 Lyr    Min II 13.0.
V0409 Lyr    P var? The elements are valid during JD2434500 - 40000.
             Blazhko effect?
V0411 Lyr    Min II 14.4. Alternatively RRC (P = 0.291315d).
V0412 Lyr    Min II 14.1; Min II - Min I = 0.48P.
V0413 Lyr    Min II 14.8?
V0415 Lyr    Cycle <= 150d.
V0417 Lyr    Min II 16.2. P var?
V0418 Lyr    P var. The elements are valid during JD2437100 - 40400.
V0423 Lyr    Min II 15.5. P var?
V0424 Lyr    Blazhko effect?
V0428 Lyr    Min II 14.3. Apsidal motion?
V0429 Lyr    Min II 14.8?
V0431 Lyr    Min II 15.1.
V0435 Lyr    Possibly ew with twice longer P. P may be spurious.
V0462 Lyr    P var? The elements are valid during JD2439913 - 40007.
V0467 Lyr    Min II 12.9. JD2415288 - 43287; the elements
             are valid during JD2415288 - 43287; large scatter
             on the light curve. According to [09412], during
             JD2443424 - 44165 the light variation range is 12.4m -
             12.6m pg, the elements are not valid.
V0470 Lyr    U = 0.40", p = 7deg. P1 = 738.6s, P2 = 557.4s, P3 = 318.0s,
             P4 = 291.9s, P5 = 259.1s.
V0473 Lyr    P var, Delta(m) var. According to [09413], P =
             1.490795d + 1.22d*10**(-6)*(JD - 2443600)/365.25d.
             Cyclic P variations: P alpha = 1178.5d; Pt = 2655d.
             Delta(m) varies with the period P alpha; P4 = 1063.5d
             may be traced in the variations of Vr.
             0.06m <= Delta(m) <= 0.36m.
V0474 Lyr    P2 = 76d.
V0477 Lyr    The central star of planetary nebula Abell 46. Strong
             reflection effect. Depths of minima: Min I 1.42m B,
             Min II ~0.1m B.
V0531 Lyr    Minima observed only between JD 2448600 and 2448800.
V0550 Lyr    SB, Porb = 1.0309d.
alf   Lyr    IR excess.
bet   Lyr    ADS 11745 A (B 8.6m, B7V, 46", 149deg; C 13.0m, 47",
             248deg). Min II 3.85. P var. Nonlinear terms:
             +3.883d*10**(-6)*E**2 - 0.10d*10**(-10)*E**3.
             Light curve shape var.
             Radio and X-ray source. IR excess.
del 2 Lyr    Open cluster delta**2 Lyr member [02505].
R     Men    Sometimes P = 120d;
             Sometimes P = 240d.
T     Men    In the Large Magellanic Cloud region; not a member of the
             Cloud. There is a sguare term in the elements:
             +8.1d*10**(-6)*E**2.
U     Men    VB A (B 10.4m, 0.6", 71deg, 1935.3). A var
             (0.8m <= A <= 2.9M). P var. Max = 2416927 + 426.9d*E
             (JD2415200 - 17400) [00207]; since JD2417400 - see Table.
V     Men    Epoch corresponds to the middle of
             the light curve ascending branch.
W     Men    The member of the Large Magellanic Cloud.
RR    Men    Min II 12.1.
RS    Men    In the Large Magellanic Cloud region; not
             a member of the Cloud.
RT    Men    In the Large Magellanic Cloud region; not a member of
             the Cloud.
RU    Men    In the Large Magellanic Cloud region; not a member of
             the Cloud.
RV    Men    In the Large Magellanic Cloud region; not a member of
             the Cloud.
RW    Men    In the Large Magellanic Cloud region; not a member of
             the Cloud.
TU    Men    Porb = 0.1176d [09376]. Superhump
             Period Ps = 0.12625d [04772].
TY    Men    Min II 8.47; d I = 0.00P, d II = 0.07P.
             Shape of the light curve varies.
TZ    Men    Min II 6.36.
UX    Men    Min II 9.47; Min II - Min I = 0.50045P.
             One of the components may be a physical variable.
WY    Men    In the region of the NGC 1841 globular cluster; not a
             member of the cluster. In the halo of the magellanic
             clouds system.
WZ    Men    In the region of the NGC 1841 globular cluster, not a
             member of the cluster. In the halo of the Magellanic
             Clouds system.
XX    Men    In the region of the NGC 1841 globular cluster, not a
             member of the cluster. In the halo of the Magellanic
             Clouds system.
XY    Men    In the Large Magellanic Cloud region; not a member of the
             Cloud. Min II 10.88; dI = 0.05P; dII = 0.00P.
XZ    Men    There are there oscillations simultaneously: P1 = 0.1083d
             (A1 = 0.0094m B), P2 = 0.0855d (A2 = 0.0082m B),
             P3 = 0.0955d (A3 = 0.0058m B); P2/P1 = 0.789.
AN    Men    Type RRC: is also possible.
iot   Men    Min II 6.05.
R     Mic    P var. Max = 2413373 + 138.60d*E (JD2413300 - 29600)
             [00458]; Max = 2432745 + 137.43d*E (JD2429600 - 34700);
             Max = 2435091 + 140.84d*E (JD2434700 - 37800);
             since JD2437800 - see Table.
S     Mic    P var. Max = 2413499 + 214.5d*E (JD2413500 - 15900) [00458];
             Max = 2432102 + 208.23d*E (JD2422700 - 32200);
             since JD2432200 - see Table.
U     Mic    OH, H2O emission.
V     Mic    OH, H20 emission.
Y     Mic    Mean brightness varies.
Z     Mic    (k - b)2 = 0.12; Delta(S) = 4.
RR    Mic    [A/H] = -1.4. P var. Max = 2433032.96 + 31.78175d*E
             (JD2415000 - 35300) [02747]; since JD2443600 - see Table.
RY    Mic    P var? Elements given in the Table represent observations
             in the interval JD2436100 - 40210.
             According to [00085] Max = 2428670 + 190d*E.
RZ    Mic    Min II 11.2.
TV    Mic    Min II 12.4.
UZ    Mic    Min II 12.4.
VW    Mic    In the interval JD2436600 - 840)
             Max = 2436807.248 + 0.35620d*E. Since JD2442600 - see
             Table.
WY    Mic    P = 0.511427d? [00001].
XZ    Mic    In the interval JD2436670 - 840 Max =
             2436731.480 + 0.449208d*E. Since JD2442630 - see Table.
ZZ    Mic    (k - b)2 = 021; Delta(S) = 0. P var? Max = 2437192.3131 +
             0.0671786d*E (JD2437180 - 460) [04308];
             Max = 2439320.2162 + 0.0671575d*E (JD2439320 - 340)
             [05683]; since JD2440440 - see Table.
             Further period increase is possible [09380]. According
             to [07985] there are two simultaneous oscillations with the
             periods P1 and P2: P1 = 0.0654d, P2 = 0.0513d.
             P2/P1 = 0.784; A2(U) = 0.25 A1(U).
AE    Mic    In the interval JD2436670 - 840 Max =
             2436728.470 + 0.324142d*E. Since JD2442630 - see Table.
AH    Mic    Min II 13.6.
AT    Mic    VB (A 10.83m V, M 4.5Ve; B 10.9m V, M 4.5Ve; a =
             6.40", P = 675 yr, e = 0.60 [09381].
             mu alpha = + 0.0216s, mu delta = -0.331" (mu, Vr,
             pi - common with AU Mic).
             Unusually high freguency of flares
             allows to suppose that both components are variable.
             The range of combined brightness variation of the
             system is given in the Table.
AU    Mic    mu alpha = +0.0212S, mu delta = -0.348" (mu, pi,
             Vr - common with AT Mic). SB? 0.20P <= M - m <= 0.55P.
             There are periodical light variations and also flares with
             A <= 0.5m U [08601].
AW    Mic    mu alpha = +0.0077s, mu delta = -0.089".
             Shape of the light curve strongly varies. Multiperiodicity
             is possible.
AX    Mic    mu alpha = -0.2805s, mu delta = -1.152". In
             minimum brightness B - V = +1.42, U - B = +1.20.
R     Mon    Peculiar non-stellar object at the apex of the reflection
             variable [09396] cometary nebula NGC 2261. Probably young
             star surrounded by dust cloud. Light curve in [09394].
S     Mon    In the open star cluster
             NGC 2264. VB A (B 8.2m, 2.9", 213deg; 9.9m, 16.6", 14deg.)
T     Mon    SB (Porb> = 70 yr [09397]). [A/H] = 0.3.
             There is a sguare term in the elements given in the
             Table: +5.34d*10**(-6)*E**2.
             Deviations from the parabola in the O - C, E diagram
             have a wave-like trend. If this wave is attributed to
             the light-time effect, Porb = 100 years.
             The observations are also satisfied by the following
             system of linear elements: Max = 2412874.56 + 27.0093d*E
             (JD2405200 - 15250) [09398]; Max = 2426004.62 + 27.0180d*E
             (JD2415250 - 27150); since JD2427150 -
             Max = 2436137.090 + 27.0205d*E [02392].
U     Mon    P var. Min = 2408897 + 92.26d*E (JD2408800 - 36210) [00368];
             since JD2437300 - see Table.
             Mean magnitude varies with the period 2320d [00657].
             Spectrum investigation [02226].
V     Mon    P var. Max = 2412172 + 334.5d*E (JD2412000 - 23500) [00458];
             Max = 2427870 + 332.5d*E (JD2423500 - 28200);
             Max = 2429904 + 342.0d*E (JD2428200 - 30800);
             Max = 2439570 + 331.6d*E (JD2430800 - 41225);
             since JD2441225 - see Table.
X     Mon    P var. Max = 2415078 + 154.0d*E (JD2415000 - 18800);
             Max = 2419758 + 149.6d*E (JD2419700 - 21000);
             Max = 2421136 + 155.0d*E (JD2421000 - 24600);
             Max = 2424673 + 169d*E (JD2424600 - 25600);
             Max = 2425644 + 155.6d*E (JD2425600 - 26800);
             Max = 2427028 + 150.7d*E (JD2427000 - 28000) [00458];
             Max = 2429521 + 155.8d*E (JD2428000 - 36300);
             Max = 2438846 + 145.3d*E (JD2437800 - 38900); since
             JD2440800 - see Table. The amplitude strongly varies;
             sometimes irregular light variations are observed.
Y     Mon    P var. Max = 2415792 + 228.6d*E (JD2415300 - 19700);
             Max = 2419928 + 227.4d*E (JD2419700 - 24300) [00458];
             Max = 2432647 + 233.3d*E (JD2424300 - 32900);
             since JD2432900 - see Table.
RR    Mon    P var. Max = 2417476 + 384.5d*E (JD2417400 - 19600) [00458];
             since JD2419600 - see Table.
RU    Mon    Min II 11.06; D II var: 0.06P <= DII <= 0.12P;
             Min II - Min I var: 0.25P < = Min II - Min I <= 0.75P.
             P var. In the interval JD2429100 - 38409 Min I =
             2418357.0140; 3.5846794d(E - 406) - 0.429d cos alpha +
             0.06d*sin(2alpha) + 0.010d*cos(3alpha) +
             0.003d*sin(4alpha), MinII = 2418355.2220 +
             3.5846794d(E - 406) + 0.429d cos alpha +
             0.060D*sin(2alpha) - 0.010d cos*3alpha +
             0.003d*sin(4alpha) (JD2416900 - 29100);
             Min I = 2429641.567 + 3.5846391d*(E - 3554) -
             0.429d*cos(alpha) + 0.060d*sin(2alpha) + 0.010d*cos(3alpha) +
             0.003d*sin(4alpha),
             Min II = 2429639.775 + 3.5846391d(E - 3554) +
             0.429d*cos(alpha) + 0.060d*sin(2alpha) -
             0.010d*cos(3alpha) + 0.003d*sin(4alpha), where alpha =
             0.01245deg(E - 406) [03445].
             The epochs E are being calculated for Min I from JD hel.
             2416901.205, and for Min II - from JD hel. 2416900.248.
             In the interval JD2438409 - 41743
             Min I = 2438409.6045 + 3.584586d(E - 6000) -
             0.4290d*cos(alpha) + 0.0620d*sin(2alpha) +
             0.0107d*cos(3alpha) + 0.0026d*sin(4alpha) -
             0.00036d cos 5alpha, Min II = 2438407.8122 +
             3.584586d(E - 6000) + 0.4290d cos alpha +
             0.0620d*sin(2alpha) - 0.0107d*cos(3alpha) +
             0.0026d*sin(4alpha) + 0.00036d*cos(5alpha),
             where alpha = 0.012385deg(E - 406) [07987].
             since JD2441743 - Min I = 2441743.2633 +
             3.584670d(E - 6930) - 0.4336d cos alpha +
             0.0634d*sin(2alpha) + 0.0111d*cos(3alpha) +
             0.0021d*sin(4alpha), Min II = 2441741.4710 +
             3.584689d(E - 6930) + 0.4336d cos alpha +
             0.0634d*sin(2alpha) - 0.0111d*cos(3alpha) +
             0.0021d*sin(4alpha), where alpha = 70.6deg +
             0.0114deg(E - 6094) [09546]. Linear elements for Min I
             epochs in 1973 - 1990 are given in the Table.
             Corresponding elements for Min II epochs are:
             Min II = 2441741.575 + 3.584567d*E. E = 0.38.
             Apsidal motion period is 285 years.
RV    Mon    Mean brightness varies with P = 1047d.
RW    Mon    Min II 9.45; d I = 0.027P, d II = 0.023P. P var.
             Min I = 2417943.687 + 1.9061012d*E (JD2417940 - 32900)
             [03450]; since JD2432900 - see Table.
RX    Mon    P var. Max = 2418980 + 343.2d*E (JD2416200 -
             19000); Max = 2423097 + 338.9d*E (JD2422000 -
             28500); since JD2428500 - see Table.
RY    Mon    VB A (B 12.29M, 28").
SS    Mon    In the region of the open cluster NGC 2264.
SU    Mon    S 5/7 - S 6/7. P var: 69d (JD2416700 - 19100); 203.5d
             (JD2420100 - 22920); 69d (JD2423000 - 30100).
             In the intervals JD2423000 - 520 - const (11.5m),
             JD2424820 - 980 - const (11.8m).
SV    Mon    [A/H] = 0.2. P var. Max = 2419041.805 + 15.230721d*E
             (JD2412000 - 22000) [00025]; Max = 2422651.931 +
             15.23256d*E (JD2422600 - 23850) [09400]; Max =
             2424571.60 + 15.2513d*E (JD2423850 - 24600);
             Max = 2434045.326 + 15.2304d*E (JD2424600 - 34100);
             since JD2433000 - see Table.
SX    Mon    Mean brightness varies with P = 1100d.
SZ    Mon    VB A (B 11m - 12m, 10" [09401]). Min II 10.55. P var.
             Min I = 2426357.1 + 32.760d*E (JD2422000 - 26400);
             Min I = 2427861.2 + 32.708d*E (JD2426750 - 32000);
             since JD2432800 - see Table.
             Shape of the light curve varies. Heights of maxima and
             depths of minima are constant.
TU    Mon    Min II 9.1.
TV    Mon    In the region of the open star cluster NGC 2237.
TW    Mon    Wachmann [03453] assigns the variable to the RRab
             type with the elements Max = 2433001.371 + 0.8743887*E,
             but notes a considerable dispersion of the points around
             the mean light curve obtained with this period. As the
             periods by Hessner (PH) and Wachmann (PW) are mutually
             related (1/PW ~1/PH + 1) it is more probable on account of
             the above mentioned circumstance that the variable belongs
             to cepheids.
TX    Mon    [A/H] = -0.3.
UV    Mon    The form of the light curve being unusual for RR Lyr type
             variables (Max II 13.5 at the phase 0.39P, Min II 13.8
             at the phase 0.22P), the period may be doubtful,
             though it was found independently by two investigators
             [00380, 03453].
UX    Mon    Min II 8.52; dI = 0.044P. P var?
             Brightness in maximum varies with the amplitude up to 0.2m.
VV    Mon    Min II 9.55; dI = dII = 0.07P.
             There is a square term in the elements given in the Table:
             -0.12d*10**(-7)*E**2.
VW    Mon    P var. Max = 2425243.40 + 0.6041350d*E (JD2414700 -
             30700); since JD2430700 - see Table.
             In [00386, 05448] And other previous works the spurious
             period value 1.532d is being accepted suggesting the
             curious nature of the variable. Serious observations are
             necessary to select the true value of the period.
VX    Mon    Depth of Min II 0.07m.
VY    Mon    In the region of the nebula IC 446.
XX    Mon    [A/H] = -0.2.
XZ    Mon    Min II 13.6; d = 0.02P:.
AA    Mon    [A/H] = -0.9. P var. Max = 2430788.266 + 3.938052d*E
             (JD2425300 - 34800) [03453]; since JD2434800 - see Table.
AC    Mon    In the region of the open cluster NGC 2323.
AK    Mon    P var. Max = 2425279 + 319.2d*E (JD2425200 - 28000); since
             JD2428000 - see Table.
AN    Mon    Min II 11.7:; d = 0.027P.
AO    Mon    Min II 10.16; DII = 0.14P; Min II - Min I = 0.4933P. P var.
             Min I = 2426735.333 + 1.884758d*E (JD2426700 - 40000);
             since JD2440000 - see Table.
AQ    Mon    Min II 10.9; DII = 0.05P; dI = 0.014P.
AR    Mon    Min II 9.03; d = 0.011P.
             There is a square term in the elements given in the Table:
             -1.22d*10**(-6)*E**2.
AU    Mon    Min II 8.2:. Shape of the light curve varies.
             Brightness in maximum varies periodically with the
             amplitude 0.2m: Max = 2443105 + 411d*E; M - m = 0.5P.
AV    Mon    Depth of Min II 0.04m.
AW    Mon    P var. Min = 2425649.053 + 20.797d*E (JD2425500 -
             26400) [09408]; Min = 2426439.340 + 20.81905d*E
             (JD2426400 - 35900) [00511]; since JD2435900 - see Table.
AX    Mon    Binary system with an envelope and gaseous streams.
             Porb = 232.60d [06103]. Spectrum investigation [09411].
             Epoch of Min brightness preceeding the moment of
             conjunction for 0.25p is given in the Table; A = 0.4m U.
             Besides periodical variations, there are rapid light
             fluctuations up to 0.1m.
BB    Mon    Depth of Min II 0.04m.
BC    Mon    P var. Max = 2421240 + 275.8d*E (JD2421200 -
             25960); Max = 2428880 + 267.2d*E (JD2425960 -
             30000); since JD2430000 - see Table.
BE    Mon    Delta(S) = 0.
BH    Mon    d = 0.01p:.
BM    Mon    Min II 12.3. According to [09415], apsidal motion is
             possible.
BO    Mon    Min II 10.1. P var. Min I = 2428211.596 + 2.2251753d*E
             (JD2415000 - 36000) [00007]; since JD2436000 - see Table.
BP    Mon    P var?
             Elements given in the Table are valid in the interval
             JD2425600 - 29700.
BT    Mon    VB A (B 16.0m, 10", 0deg).
             After the outburst in 1939 the brightness varies in the
             range 16.0m - 18.7m with the elements: Min =
             2443491.7155 + 0.3338141d*E; D = 0.20p, 0 <= d < = 0.03p.
             Before the outburst in 1939, according to [09417],
             the following elements were valid: Min = 2429500.207 +
             0.3338010d*E. Emission nebula with the radius of 3.8"
             was discovered in 1981 around the nova [09148].
BX    Mon    Usually was considered as mira type variable
             [09421]. In the Table the epoch of light maximum and
             the period are given according to [09419]. According
             to [09420] the Balmer emission lines originate in the
             nebulosity surrounding the symbiotic system and are
             excited by the hot component, and light variations
             are due to the orbital motion in the system.
BZ    Mon    d = 0.030P. In the region of the open cluster CR 106.
CC    Mon    In the region of the open cluster CR 106.
CD    Mon    P var. Max = 2427704 + 273.8d*E (JD2427400 - 30400); since
             JD2430400 - see Table.
CE    Mon    Min II 14.2.
CF    Mon    Min II 13.7; d = 0.02P:.
CH    Mon    d = 0.030P.
CS    Mon    VB A (B 13m, 9", 0deg).
CT    Mon    In the region of the open cluster NGC 2244.
CU    Mon    [A/H] = -0.2.
CV    Mon    In the centre of an anonymous open cluster.
             VB A (B 13.76m, 10", 270deg; C 13.72m, 14", 270deg).
             P var. Max = 2429805.142 + 5.378782d*E (JD2429360 -
             36000); since JD2436000 - see Table.
DD    Mon    Min II 11.3.
DF    Mon    The chart in [05285] is wrong, the star observed was
             not DF Mon.
DN    Mon    Min II 13.9.
DR    Mon    In the region of the open cluster Cr 106.
DT    Mon    P var. Max = 2425324 + 345d*E (JD2425300 - 28200)
             In the interval JD2429250 - 37700 there were cycles 119d,
             230d, 350d.
DW    Mon    In the region of the open cluster NGC 2286.
EE    Mon    P var. Max = 2425300.42 + 4.80776d*E (JD2425300 -
             27720); since JD2427720 - see Table.
EH    Mon    d = 0.023P.
EK    Mon    P var. Max = 2425302.59 + 3.95773d*E (JD2425200 -
             33000) [00387]; since JD2433000 - see Table.
EP    Mon    d = 0.026P.
ES    Mon    d = 0.02P.
EW    Mon    Min II 14.2.
FH    Mon    Depth of Min II 0.04m.
FP    Mon    In the region of the open cluster NGC 2353.
FS    Mon    Min II 11.2.
FU    Mon    S 6.5/7.5.
FW    Mon    d = 0.016P. Depth of Min II 0.04m.
FX    Mon    OH emission.
FZ    Mon    The elements should be checked.
GH    Mon    Min II 13.1.
GP    Mon    In the region of the open cluster NGC 2264.
GQ    Mon    In the region of the open cluster NGC 2264.
GR    Mon    In the region of the open cluster NGC 2264.
GU    Mon    Min II 12.5.
GV    Mon    Depth of Min II 0.04m.
GX    Mon    OH, H2O, SIO maser.
HI    Mon    Min II 9.9.
HM    Mon    Min II 13.6. P var. Min I = 2430110.1948 + 0.40765737d*E
             (JD2429600 - 35400) [05285]; since JD2435400 - see Table.
HO    Mon    d = 0.03P.
HP    Mon    d = 0.04P:.
HR    Mon    Depth of Min II 0.03m.
HY    Mon    Min II 12.4.
IL    Mon    d = 0.03P.
IM    Mon    Min II 6.47.
IO    Mon    In the region of the open cluster NGC 2264.
IP    Mon    In the region of the open cluster NGC 2264.
IQ    Mon    In the region of the open cluster NGC 2264.
IR    Mon    P var?
IS    Mon    Depth of Min II 0.05m.
IX    Mon    Min II 12.8.
IZ    Mon    Min II 12.0.
KU    Mon    In the region of the open cluster NGC 2264.
KV    Mon    In the region of the open cluster NGC 2264.
KW    Mon    In the region of the open cluster NGC 2264.
KX    Mon    In the region of the open cluster NGC 2264.
KY    Mon    In the region of the open cluster NGC 2264.
KZ    Mon    In the region of the open cluster NGC 2264.
LL    Mon    In the region of the open cluster NGC 2264.
LM    Mon    In the region of the open cluster NGC 2264.
LN    Mon    In the region of the open cluster NGC 2264.
LO    Mon    In the region of the open cluster NGC 2264.
LP    Mon    In the region of the open cluster NGC 2264.
LQ    Mon    In the region of the open cluster NGC 2264.
LR    Mon    In the region of the open cluster NGC 2264.
LS    Mon    In the region of the open cluster NGC 2264.
LT    Mon    In the region of the open cluster NGC 2264.
LU    Mon    In the region of the open cluster NGC 2264.
LV    Mon    In the region of the open cluster NGC 2264.
LW    Mon    In the region of the open cluster NGC 2264.
LX    Mon    In the region of the open cluster NGC 2264.
LY    Mon    In the region of the open cluster NGC 2264.
LZ    Mon    In the region of the open cluster NGC 2264.
MM    Mon    In the region of the open cluster NGC 2264.
MN    Mon    In the region of the open cluster NGC 2264.
MO    Mon    VB A (B 20m, 10", 356deg); in the region of the
             open cluster NGC 2264.
MP    Mon    In the region of the open cluster NGC 2264.
MQ    Mon    In the region of the open cluster NGC 2264.
MX    Mon    Min II 11.7.
NN    Mon    Min II 12.9.
NS    Mon    Min II 11.1.
NT    Mon    In the region of the open cluster NGC 2264.
NU    Mon    In the region of the open cluster NGC 2264.
NV    Mon    In the region of the open cluster NGC 2264.
NW    Mon    In the region of the open cluster NGC 2264.
NX    Mon    In the region of the open cluster NGC 2264.
NY    Mon    In the region of the open cluster NGC 2264.
NZ    Mon    In the region of the open cluster NGC 2264.
OO    Mon    In the region of the open cluster NGC 2264.
OP    Mon    In the region of the open cluster NGC 2264.
OQ    Mon    In the region of the open cluster NGC 2264.
OR    Mon    In the region of the open cluster NGC 2264.
OS    Mon    In the region of the open cluster NGC 2264.
OT    Mon    In the region of the open cluster NGC 2264.
OU    Mon    In the region of the open cluster NGC 2264.
OV    Mon    In the region of the open cluster NGC 2264.
OW    Mon    In the region of the open cluster NGC 2264.
OX    Mon    VB A (B 15m, 7", 35deg); in the region of the open
             cluster NGC 2264.
OY    Mon    In the region of the open cluster NGC 2264.
OZ    Mon    In the region of the open cluster NGC 2264.
PP    Mon    In the region of the open cluster NGC 2264.
PQ    Mon    In the region of the open cluster NGC 2264.
PR    Mon    The elements should be checked.
PT    Mon    In the region of the open cluster NGC 2264.
PU    Mon    In the region of the open cluster NGC 2264.
PV    Mon    In the region of the open cluster NGC 2264.
PW    Mon    In the region of the open cluster NGC 2264.
PX    Mon    In the region of the open cluster NGC 2264.
PY    Mon    In the region of the open cluster NGC 2264.
QR    Mon    290d <= P <= 400d. Depth of Min varies by
             0.9m with the period about 2000d.
QT    Mon    In the region of the open cluster NGC 2264.
QU    Mon    In the region of the open cluster NGC 2264.
QV    Mon    In the region of the open cluster NGC 2264.
QW    Mon    In the region of the open cluster NGC 2264.
QX    Mon    In the region of the open cluster NGC 2264.
QY    Mon    In the region of the open cluster NGC 2264.
QZ    Mon    In the region of the open cluster NGC 2264.
V0334 Mon    In the region of the open cluster NGC 2264.
V0335 Mon    In the region of the open cluster NGC 2264.
V0336 Mon    In the region of the open cluster NGC 2264.
V0337 Mon    In the region of the open cluster NGC 2264.
V0338 Mon    In the region of the open cluster NGC 2264.
V0339 Mon    In the region of the open cluster NGC 2264.
V0340 Mon    In the region of the open cluster NGC 2264.
V0341 Mon    In the region of the open cluster NGC 2264.
V0342 Mon    In the region of the open cluster NGC 2264.
V0343 Mon    In the region of the open cluster NGC 2264.
V0344 Mon    In the region of the open cluster NGC 2264.
V0345 Mon    In the region of the open cluster NGC 2264.
V0346 Mon    In the region of the open cluster NGC 2264.
V0347 Mon    VB A (B 20m, 12", 120deg); in the region of the open
             cluster NGC 2264.
V0348 Mon    In the region of the open cluster NGC 2264.
V0349 Mon    In the region of the open cluster NGC 2264.
V0350 Mon    In the region of the open cluster NGC 2264.
V0351 Mon    In the region of the open cluster NGC 2264.
V0352 Mon    In the region of the open cluster NGC 2264.
V0353 Mon    In the region of the open cluster NGC 2264.
V0354 Mon    In the region of the open cluster NGC 2264.
V0355 Mon    In the region of the open cluster NGC 2264.
V0356 Mon    VB (3", 78deg); in the region of the open cluster
             NGC 2264.
V0357 Mon    In the region of the open cluster NGC 2264.
V0358 Mon    In the region of the open cluster NGC 2264.
V0359 Mon    In the region of the open cluster NGC 2264.
V0360 Mon    In the region of the open cluster NGC 2264.
V0361 Mon    In the region of the open cluster NGC 2264.
V0362 Mon    In the region of the open cluster NGC 2264.
V0363 Mon    In the region of the open cluster NGC 2264.
V0364 Mon    In the region of the open cluster NGC 2264.
V0365 Mon    VB B (A = V591 Mon, B 7", 135deg); in the region of the
             open cluster NGC 2264.
V0366 Mon    In the region of the open cluster NGC 2264.
V0367 Mon    In the region of the open cluster NGC 2264.
V0368 Mon    VB (9", 252deg); in the region of the open cluster
             NGC 2264.
V0369 Mon    VB (11", 264deg); in the region of the open cluster
             NGC 2264.
V0370 Mon    VB (8", 97deg); in the region of the open cluster
             NGC 2264.
V0371 Mon    In the region of the open cluster NGC 2264.
V0372 Mon    SC 7/7.5.
V0373 Mon    In the region of the open cluster NGC 2264.
V0379 Mon    d = 0.015P:.
V0380 Mon    Min II 12.9; P = 1.98904166d?
V0383 Mon    Min II 15.2.
V0384 Mon    Min II 13.0.
V0389 Mon    Min II 14.9.
V0393 Mon    Min II 14.3.
V0394 Mon    d = 0.02P; depth of Min II 0.04m.
V0395 Mon    d = 0.03P.
V0396 Mon    Min II 13.5.
V0397 Mon    Min II 11.9.
V0398 Mon    In the region of the open cluster NGC 2264.
V0399 Mon    In the region of the open cluster NGC 2264.
V0400 Mon    In the region of the open cluster NGC 2264.
V0401 Mon    In the region of the open cluster NGC 2264.
V0402 Mon    In the region of the open cluster NGC 2264.
V0403 Mon    In the region of the open cluster NGC 2264.
V0404 Mon    d = 0.02P:.
V0405 Mon    In the region of the open cluster NGC 2264.
V0406 Mon    In the region of the open cluster NGC 2264.
V0407 Mon    In the region of the open cluster NGC 2264.
V0408 Mon    In the region of the open cluster NGC 2264.
V0409 Mon    In the region of the open cluster NGC 2264.
V0410 Mon    In the region of the open cluster NGC 2264.
V0411 Mon    In the region of the open cluster NGC 2264.
V0412 Mon    In the region of the open cluster NGC 2264.
V0413 Mon    In the region of the open cluster NGC 2264.
V0414 Mon    In the region of the open cluster NGC 2264.
V0415 Mon    In the region of the open cluster NGC 2264.
V0416 Mon    In the region of the open cluster NGC 2264.
V0417 Mon    In the region of the open cluster NGC 2264.
V0418 Mon    In the region of the open cluster NGC 2264.
V0419 Mon    In the region of the open cluster NGC 2264.
V0420 Mon    In the region of the open cluster NGC 2264.
V0421 Mon    In the region of the open cluster NGC 2264.
V0422 Mon    In the region of the open cluster NGC 2264.
V0423 Mon    In the region of the open cluster NGC 2264.
V0424 Mon    In the region of the open cluster NGC 2264.
V0425 Mon    In the region of the open cluster NGC 2264.
V0426 Mon    VB A (B = NSV 3125 17.0m, 6", 117deg); in the region of
             the open cluster NGC 2264.
V0427 Mon    In the region of the open cluster NGC 2264.
V0428 Mon    In the region of the open cluster NGC 2264.
V0429 Mon    In the region of the open cluster NGC 2264.
V0430 Mon    In the region of the open cluster NGC 2264.
V0431 Mon    In the region of the open cluster NGC 2264.
V0432 Mon    In the region of the open cluster NGC 2264.
V0433 Mon    In the region of the open cluster NGC 2264.
V0434 Mon    In the region of the open cluster NGC 2264.
V0435 Mon    In the region of the open cluster NGC 2264.
V0436 Mon    In the region of the open cluster NGC 2264.
V0437 Mon    In the region of the open cluster NGC 2264.
V0438 Mon    In the region of the open cluster NGC 2264.
V0439 Mon    In the region of the open cluster NGC 2264.
V0440 Mon    In the region of the open cluster NGC 2264.
V0441 Mon    In the region of the open cluster NGC 2264.
V0442 Mon    Min II 11.6.
V0443 Mon    In the region of the open cluster NGC 2264.
V0444 Mon    In the region of the open cluster NGC 2264.
V0445 Mon    Min II 11.3.
V0446 Mon    [A/H] = -0.7.
V0447 Mon    [A/H] = -1.4.
V0448 Mon    Min II 9.8.
V0449 Mon    d = 0.02P.
V0450 Mon    Min II 12.6.
V0451 Mon    Min II 14.7.
V0452 Mon    Min II 12.7; d = 0.02P.
V0453 Mon    Min II 11.8.
V0454 Mon    Min II 12.2.
V0455 Mon    Min II 15.3.
V0456 Mon    Min II 13.7.
V0457 Mon    Min II 14.3; d = 0.03P:.
V0458 Mon    Min II 13.8.
V0459 Mon    Min II 14.7.
V0460 Mon    Min II 10.7.
V0463 Mon    d = 0.03P; P = 2.2476768d?
V0464 Mon    Min II 12.3.
V0465 Mon    P var. Max = 2429642.44 + 2.71341d*E (JD2425600 -
             30800) [03551]; Max = 2431845.65 + 2.713212d*E
             (JD2430000 - 35200) [03453]; Max = 2435541.315 +
             2.713668d*E (JD2435200 - 41600); since JD2441600 - see
             Table.
V0466 Mon    VB A (B 15m, 135deg).
V0474 Mon    (k - b)2 = 0.32. Blazhko effect:
             Max(O - C) = 2441664.962 + 7.74639d*N; Min(O - C) =
             2441669.569 + 7.74639d*N; 0.03m <= A <= 0.37m;
             -0.02d <= O - C <= +0.03d. Freguency analysis gives
             three principal oscillations [08669]: P1 = 0.1361258d
             (A1 = 0.18m), P2 = 0.1337745d (A2 = 0.12m),
             P3 = 0.1385591d (A3 = 0.04m).
V0478 Mon    In the region of the nebula IC 2169.
V0479 Mon    In the region of the nebula IC 2169.
V0481 Mon    In the region of the nebula IC 2169.
V0482 Mon    In the region of the nebula IC 2169.
V0483 Mon    In the region of the nebula IC 2169.
V0486 Mon    VB A (B 18.4M, 6"). In the region of the nebula NGC 2245.
V0487 Mon    In the region of the nebula NGC 2245.
V0488 Mon    In the region of the nebula NGC 2245.
V0489 Mon    In the region of the nebula NGC 2245.
V0490 Mon    In the region of the nebula NGC 2247.
V0493 Mon    In the region of the open cluster Tr 5.
V0494 Mon    Depth of Min II 0.05m.
V0496 Mon    Min II 12.8.
V0497 Mon    8.9 - 11.8 IR.
V0498 Mon    P = 2.4727818d?
V0500 Mon    In the region of the open cluster NGC 2264.
V0501 Mon    Min II 13.1; Min II - Min I = 0.445P; DII = 0.036P.
V0503 Mon    9.2 - 10.9 IR.
V0505 Mon    Min II 7.55.
V0507 Mon    SB2 (P = 53.781d [09483]); d = 0.015P:.
V0510 Mon    [A/H] = -0.1.
V0513 Mon    Depth of Min II 0.04m.
V0514 Mon    Min II 13.3.
V0515 Mon    Min II 12.7.
V0521 Mon    Min II 10.4.
V0524 Mon    Min II 15.2.
V0526 Mon    P var. Max = 2433304.284 + 2.675208d*E (JD2429300 -
             35170); since JD2439170 - see Table.
V0527 Mon    Depth of Min II 0.05m.
V0530 Mon    Min II 12.8.
V0532 Mon    Min II 12.8. RRC?
V0535 Mon    P var. Max = 2431846.445 + 0.3328791d*E
             (JD2429600 - 34060); since JD2434060 - see Table.
             [Fe/H] = -1.44.
V0539 Mon    In the region of the open cluster NGC 2244.
V0540 Mon    In the region of the nebula IC 446.
V0541 Mon    In the region of the nebula IC 446.
V0542 Mon    In the region of the nebula IC 446.
V0543 Mon    In the region of the open cluster NGC 2244.
V0544 Mon    In the region of the open cluster NGC 2244.
V0545 Mon    In the region of the open cluster NGC 2244.
V0546 Mon    In the region of the open cluster NGC 2244.
V0547 Mon    In the region of the open cluster NGC 2244.
V0548 Mon    In the region of the open cluster NGC 2244.
V0549 Mon    In the region of the open cluster NGC 2244.
V0550 Mon    VB A (B 17.3m, 6", 0deg ); in the region of the open
             cluster NGC 2244.
V0551 Mon    In the region of the open cluster NGC 2244.
V0552 Mon    In the region of the open cluster NGC 2244.
V0553 Mon    In the region of the open cluster NGC 2244.
V0554 Mon    In the region of the open cluster NGC 2244.
V0555 Mon    In the region of the open cluster NGC 2244.
V0556 Mon    In the region of the open cluster NGC 2244.
V0557 Mon    In the region of the open cluster NGC 2244.
V0560 Mon    Depth of Min II 0.05m.
V0565 Mon    Connected with the diffuse nebula
             NGC 2313 having diameter of 10" and a faint cometary
             nebula.
V0569 Mon    VB A (B 10.8m, 6.2", 281deg; C 10.5m, 38.3", 295deg).
             The range of combined light variation of A and B
             components is given. According to [08215], P = 0.18d.
V0571 Mon    (k - b)2 = 0.32.
             Non-radial pulsation with variable periods:
             P1 = 0.0999081d (A1 = 0.052m), P2 = 0.0749998d
             (A2 = 0.015m) (JD2440914 - 41692) [07127]; P1 = 0.0894534d
             (A1 = 0.038m), P2 = 0.15988d (A2 = 0.025m), P3 = 0.106516d
             (A3 = 0.014m). P4 = 0.26998d (A4 = 0.012m), P5 = 0.15069d
             (A5 = 0.011m) (JD2441662 - 719) [09450].
V0577 Mon    VB (A 11.3m V, B 14.8m V; a = 0.312", P = 16.60 yr, e =
             0.38); mu alpha = +0.049S, mu beta = +0.73".
             Both components are probably variables. The range
             of combined light variation of the system is given
             in the Table [06146].
V0578 Mon    In the region of the open cluster NGC 2244.
V0579 Mon    In the region of the open cluster NGC 2264.
V0580 Mon    In the region of the open cluster NGC 2264.
V0581 Mon    In the region of the open cluster NGC 2264.
V0582 Mon    In the region of the open cluster NGC 2264.
V0583 Mon    In the region of the open cluster NGC 2264.
V0584 Mon    In the region of the open cluster NGC 2264.
V0585 Mon    In the region of the open cluster NGC 2264.
V0586 Mon    In the region of the open cluster NGC 2264.
V0588 Mon    In the region of the open cluster NGC 2264.
V0589 Mon    In the region of the open cluster NGC 2264.
V0590 Mon    VB (10", 358deg); in the region of the open cluster
             NGC 2264.
V0591 Mon    VB A (B = V365 Mon, 7", 135deg); in the region of the open
             cluster NGC 2264.
V0593 Mon    In the region of the open cluster NGC 2264.
V0594 Mon    In the region of the open cluster NGC 2264.
V0595 Mon    In the region of the open cluster NGC 2264.
V0596 Mon    In the region of the open cluster NGC 2264.
V0597 Mon    In the region of the open cluster NGC 2264.
V0598 Mon    In the region of the open cluster NGC 2264.
V0599 Mon    In the region of the open cluster NGC 2264.
V0600 Mon    In the region of the open cluster NGC 2264.
V0601 Mon    In the region of the open cluster NGC 2264.
V0602 Mon    In the region of the open cluster NGC 2264.
V0603 Mon    In the region of the open cluster NGC 2264.
V0604 Mon    In the region of the open cluster NGC 2264.
V0605 Mon    In the region of the open cluster NGC 2264.
V0606 Mon    In the region of the open cluster NGC 2264.
V0607 Mon    In the region of the open cluster NGC 2264.
V0608 Mon    In the region of the open cluster NGC 2264.
V0609 Mon    In the region of the open cluster NGC 2264.
V0610 Mon    In the region of the open cluster NGC 2264.
V0611 Mon    In the region of the open cluster NGC 2264.
V0612 Mon    In the region of the open cluster NGC 2264.
V0613 Mon    S 3/2.
V0616 Mon    Novalike outbursts were observed in 1917 (Max JD2421540)
             and in 1975 (Max JD2442646). In quiescent state probably
             ellipsoidal light variation is observed with P = 0.325d
             and A = 0.2m [09458], and also slower light variations
             with P = 7.39d [09459] or 7.8d [09460]. Spectrum description
             [09461, 09462].
V0624 Mon    In the region of the open cluster Cr 106.
V0628 Mon    In the region of the open cluster NGC 2264.
V0629 Mon    In the region of the open cluster NGC 2264.
V0630 Mon    VB A (B 21m, 3", 300deg); in the region of the open
             cluster NGC 2264.
V0632 Mon    In the region of the open cluster NGC 2368.
V0637 Mon    Basic oscillation with A1 = 0.05m and elements given in
             the Table is superimposed by the second one with
             A2 = 0.02m and the elements: Max = 2443496.1624 +
             0.19740d*E. Beat period Pb = 6.09d.
V0638 Mon    VB (6.5m, 8.5m; 0.8", 178deg).
V0640 Mon    In the region of the open cluster NGC 2244.
             Porb = 14.39604d [06103].
             Irregular light variations.
             Probably transitional stage from a binary system of
             O stars to a system of WR type [04107].
V0641 Mon    VB A (B 10.91m, 21.4", 310deg; C 12.46m, 25.8", 285deg).
             In the region of the open cluster NGC 2264.
V0642 Mon    In the region of the open cluster NGC 2264. Cluster
             non-member. Epoch of light minimum is
             given in the Table.
V0645 Mon    Epoch of light minimum is given in the Table.
V0741 Mon    Type ACV: is also possible.
V0750 Mon    In the region of the nebula IC 2177.
V0753 Mon    Type ACV: is also possible.
S     Mus    Marked on the chart for BO Mus. Max II = Max I,
             ” (Max II) = 0.15P. P var? SB 1 (Porb = 506.4d).
T     Mus    P2 = 1021d.
V     Mus    In the Coal Sack region.
RV    Mus    P = 128d: is possible.
RW    Mus    P = 130d: is possible.
RY    Mus    V1 (NGC 4833).
RZ    Mus    V2 (NGC 4833). Cluster non-member.
SY    Mus    Min II 11.2; Min I - Min II = 170d.
             Elements for Min I of quasiperiodic variations observed
             during JD2434910 - 41510 are given. Radio source.
TU    Mus    Min II 8.65. P var. Min I = 2424260.396 + 1.38728d*E
             (JD2423900 - 29300) [00039]; during JD2437380 - 41900 - see
             Table. The light curve shape var.
TV    Mus    Min II 11.3.
TW    Mus    Min II 12.4.
TZ    Mus    B - V: +1.22, +1.43.
UW    Mus    Min II 11.9.
UY    Mus    Min II 12.0.
VW    Mus    Min II 13.9.
WY    Mus    P var. Periodic term: +0.35d*sin(0.12deg*E).
XZ    Mus    Before JD2419200 Max = 2412590 + 113d*E.
AB    Mus    Min II 13.0.
AS    Mus    [A/H] = 0.5.
AX    Mus    P var. During JD2412550 - 19200 - see Table; during
             JD2423900 - 26100 P = 97.3d.
AY    Mus    Min II 10.8. Min II - Min I = 0.481P.
             The elements are valid during 1897 - 1943. In the time
             interval JD2441683 - 721 eclipses did not occur [08094].
BB    Mus    P, possibly P should be doubled.
BD    Mus    Depth of Min II 0.05m.
BE    Mus    Min II 14.1.
BF    Mus    Min II 14.4.
BK    Mus    P very long P: 56d < d < 310d.
BR    Mus    Min II 11.25. B - V: +0.10m.
BS    Mus    Min II 11.5.
BX    Mus    Depth of Min II 0.04m.
CD    Mus    Min II 14.7.
CS    Mus    P > 120d.
DW    Mus    According to [08135], the spectral type is M5e, typical of
             Mira stars. Elements in [03934] were deduced from the
             observed brightness variations with P ~355d which
             was considered to be a spurious period; rapid variations
             were confirmed by 7h of photographic observations.
DZ    Mus    Possibly Pshould be doubled.
EE    Mus    In the coal sack. The flare was observed spectroscopically.
EN    Mus    d = 0.035P:.
EP    Mus    [A/H] = 0.2. According to [08136], EA,
             P = 4.15d, D = 0.05P, 11.63m - 12.60m V, Min II 11.7:.
ET    Mus    Alternatively possible type EW [08727, 04001].
EV    Mus    d = 0.09P:.
EY    Mus    In the Coal Sack region.
EZ    Mus    Alternative possible values of P 4.3032d, 4.3224d.
FH    Mus    Depth of Min II 0.03m.
FO    Mus    P var?
GK    Mus    Min II 15.0.
GN    Mus    Min II 14.2.
GO    Mus    Min II 15.2.
GP    Mus    B - V: +1.03, +1.61.
KU    Mus    Type RV: is also possible.
alf   Mus    VB A (B 13.0m, 29.3", 316deg).
eta   Mus    VB A (B 7.30m, 60").
tet   Mus    VB (A 5.64m, B 7.5m, 5.3", 187deg); SB (Porb = 18.341B).
             Variable intensity of emission lines with respect to the
             continuum (double wave; elements in the Table are for the
             epochs of Min I variability in the UV range (lambda lambda
             1550 - 3300 A) with an amplitude about 2%, P = 1.5d and
             rapid changes (lamda lamda 1550 - 1800 A) with an
             amplitude about 3 - 5% on the time scale of 50s - 70s
             [08532]. Connected with a nebula, 80'*45'.
R     Nor    VB A (B 14.0m, 5.7", 268deg, 1929). P var. Max II =
             2406371 + 486.94d*E (JD2406300 - 25000); Max II =
             2426359 + 500.56d*E (JD2426000 - 30500); Max II =
             2431377 + 489.0d*E (JD2430500 - 34500); since
             JD2437600 - see Table. Like R Cen, has a doudle Max,
             JD2437600 - see Table. Like R Cen, has a doudle Max,
             divided by a comparatively shallow Min II. Max II is
             usually brighter than Max I. ” (Min I) = 0.43P,
             ” (Max I) = 0.70P, ”(Min II) = 0.85P.
S     Nor    In the centre of the open cluster NGC 6087, cluster member.
             [A/H] = -0.1.
T     Nor    P var.Max = 2414783 + 241.87d*E (JD2414700 - 28000);
             Max = 2428084 + 244.93d*E (JD2428000 - 35000);
             since JD2437000 - see Table.
U     Nor    P var. Max = 2415028.94 + 12.64084d*E (JD2415000 - 26000)
             [00060]; since JD2434000 - see Table, [A/H] = -0.6.
W     Nor    P2 ~1300d.
Y     Nor    VB A (B 12.2m vis, 4.0", 156deg, 1903).
Z     Nor    Min II 9.6.
RR    Nor    Min II 9.9.
RS    Nor    B - V: +1.13,  +1.48.
RT    Nor    Quasiperiodic variations: P1 ~59d, P2 ~175d [08140].
RV    Nor    [A/H] = 0.8.
             There are irregularities in the light curve.
SV    Nor    Min II 12.6.
SW    Nor    d = 0.003P.
SX    Nor    d = 0.1P.
SY    Nor    VB A (B 12.8m, 2.1", 315deg, 1934). B - V: +1.16,  +1.49.
             [A/H] = 0.5.
SZ    Nor    Min II 12.6.
TT    Nor    Twice longer P is possible.
TU    Nor    Min II 12.5. Associated with a small faint nebula.
TV    Nor    Min II 9.3.
TW    Nor    In the region of the poor open cluster Lynga 6.
             B - V: +1.79, +2.22. [A/H] = 0.2.
TX    Nor    Min II 12.5.
TZ    Nor    Min II 12.1.
UV    Nor    d ~0.07P.
UX    Nor    In Max light B - V = +0.30.
UY    Nor    d = 0.025P.
UZ    Nor    d = 0.02P.
VV    Nor    In the region of the cluster NGC 6152.
VX    Nor    Depth of Min II ~0.03m.
VZ    Nor    In the region of the cluster NGC 6152. Min II 14.3.
WX    Nor    The chart is erroneously labelled as that for WZ Nor.
             Min II 12.8.
WZ    Nor    The chart is erroneously labelled as that for WX Nor.
             Min II 13.4.
XY    Nor    Min II 13.2.
AA    Nor    [A/H] = -0.1.
AF    Nor    In the region of the open cluster NGC 5999.
AQ    Nor    The chart in [06286] is wrong.
AR    Nor    The chart in [06286] is wrong.
AT    Nor    d = 0.026P:.
BE    Nor    Min II 14.2.
BF    Nor    The chart in [06286] is wrong.
BH    Nor    Min II 13.2.
BP    Nor    Close companion.
CE    Nor    d = 0.05P. Min II 11.8?
CG    Nor    The chart in [06286] is wrong.
CI    Nor    The chart in [06286] is wrong.
CT    Nor    The chart in [06286] is wrong.
CX    Nor    Min II 15.0.
DE    Nor    The chart in [06286] is wrong.
DF    Nor    The chart in [06286] is wrong.
DO    Nor    Min II 14.2. In the region of the open cluster NGC 6087.
DP    Nor    The chart in [06286] is wrong.
DR    Nor    In the region of the open cluster NGC 6087.
EE    Nor    The chart in [06286] is wrong.
EM    Nor    Min II 13.8.
ET    Nor    d = 0.032P.
FG    Nor    The chart in [06286] is wrong.
FI    Nor    The chart in [06286] is wrong.
FK    Nor    Min II 15.0.
FQ    Nor    According to [00060], P = 1.994d?
FW    Nor    Min II 14.5.
GM    Nor    d = 0.02P; Min II 11.01; Min II - Min I = 0.499P
             (JD2441683 - 721), Min II - Min I = 0.531P (JD2425381 -
             28402). B - V = 0.44m.
GN    Nor    Min II 13.3, DII = 0.16P, Min II - Min I = 0.405P
             (JD2425900). Apsidal motion: P = 500yr.
GO    Nor    Min II 13.7.
GQ    Nor    Min II 13.8.
GR    Nor    [A/H] = 0.9.
GT    Nor    d = 0.048P.
GU    Nor    In the region of the open cluster NGC 6067.
             B - V: +1.17, +1.40. [A/H] = 0.1.
GV    Nor    d = 0.03P:.
GX    Nor    Min II 15.0.
HH    Nor    VB B (A 9.9m vis, FO; B 12.6", 148deg). d = 0.05P.
HI    Nor    D is very small.
HK    Nor    Min II 12.9.
HO    Nor    Min II 13.2:.
HW    Nor    d = 0.024P.
HZ    Nor    P = 2.921584d is possible.
IQ    Nor    B - V: +1.55, +1.93.
IS    Nor    In the region of the open cluster NGC 6067.
IT    Nor    Min II 9.8.
KL    Nor    P >= 140d.
KM    Nor    P >= 170d.
KQ    Nor    Mira Ceti type is not excluded [04001].
KT    Nor    P >= 180d.
KX    Nor    Min II 14.8.
LO    Nor    P >= 220d.
LV    Nor    Deep Min II.
LX    Nor    Possible P values: 0.60492d, 0.7851d, etc.
NR    Nor    Min II 15.9.
NW    Nor    P > 140d.
NX    Nor    Min II 14.4.
OS    Nor    Epoch of Min is given. EW/KW type is possible.
OT    Nor    Min II 13.7.
OU    Nor    Min II 15.1.
OV    Nor    P >= 200d.
OW    Nor    P >= 120d.
OX    Nor    P >= 110d.
PQ    Nor    Possibly a cepheid which is a fainter component of an
             unresolved binary. Epoch of Max is given.
PT    Nor    In the region of the open cluster NGC 6067.
QT    Nor    HV 5388 = HV 8903. The coordinates in [00424] are wrong.
QV    Nor    3U 1538 - 52. No.12 [04124].
             Epoch of Min corresponding to the X-ray eclipse is given.
             Depth of Min I 0.05m V, that of Min II 0.08m V. The period
             of X-ray pulses Px = 528.928s [04114]. A flare was observed
             with Delta(m) > 0.3m [09456].
QX    Nor    4U 1608 - 52.
QZ    Nor    In the open cluster NGC 6067.
V0367 Nor    May be not a supergiant.
V0374 Nor    Type LBV: is also possible.
mu    Nor    In the region of the open cluster NGC 6169.
U     Oct    P var. Max = 2420685 + 302.00d*E (JD2414900 -
             20700); Max = 2424320 + 300.74d*E (JD2422800 -
             29800); Max = 2431901 + 309.60d*E (JD2429800 -
             32250); Max = 2434018 + 300.70d*E (JD2432250 -
             38800); since JD2438800 - see Table.
X     Oct    P var.Max = 2415170 + 208.40d*E (JD2415100 -
             17100); Max = 2417425 + 201.24d*E (JD2417100 -
             20700); Max = 2423780 + 207.95d*E (JD2422000 -
             24000); Max = 2424370 + 200.18d*E (JD2424000 -
             25600); since JD2425600 - see Table. Depths of minima are
             stongly variable; 1.1m <= A <= 4.0m.
RV    Oct    Delta(S) = 10.
TX    Oct    Min II 12.7.
UV    Oct    Delta(S) = 9; (k - b)2 = 0.06. Blazhko effect: P = 80d;
             0.14P <= M - m <= 0.24P, 0.4m <= A <= 1.3m.
UZ    Oct    Min II 9.48; dI = 0.00P, dII = 0.05P. P var. Min I =
             2440223.1560 + 1.1493709d*E (JD2438300 - 42000);
             since JD2442000 - see Table.
AM    Oct    Min II 14.9.
BE    Oct    P < 20d:.
BG    Oct    P = 0.7490d?
BK    Oct    Min II 14.6.
BP    Oct    (k - b)2 = 0.25.
CC    Oct    Basic radial pulsation with P1 = 0.12490d (A1 = 0.042m)
             is superimposed by others with periods: P2 = 0.0795317d
             (A2 = 0.008m), P3 = 0.12336d (A3 = 0.014m); P4 =
             0.11068d (A4 = 0.008m), P5 = 0.12713d (A5 = 0.006m);
             P6 = 0.11815d (A6 = 0.006m).
CD    Oct    mu = 0.51", p = 279deg. One of the periods P = 686s
             (A = 0.01m).
CE    Oct    Light oscillation with P2 = 0.054511d (A2 = 0.0056m) is
             superimposed by an oscillation with P1 = 0.2100d or
             0.2660d (A1 = 0.0052m), which is due to pulsation or
             ellipsoidal variability in a close binary system.
CP    Oct    Variability type and spectral type (F2/F3Ib/II) do not agree.
alf   Oct    SB, Porb = 9.073d.
R     Oph    P var. Max = 2399214 + 302.1d*E (JD2399200 - 2427900)
             [00458]; Max = 2427915 + 304.0d*E (JD2427900 - 34900);
             Max = 2434906 + 301.5d*E (JD2434900 - 40600) [00001];
             since JD2440600 - see Table.
U     Oph    ADS 10428 A (B 12.26m, GOV, 20.4", 358deg). Min II 6.46.
             P var. Periodic term:
             +0.0120d*sin(0.0483deg*E + 4.7833deg).
V     Oph    P var. Max = 2411155 + 296.73d*E (JD2411000 - 24000);
             Max = 2424198 + 302.46d*E (JD2424000 - 28000);
             since JD2428000 - see Table.
W     Oph    P var. Before JD2420500 Max = 2415186 +
             335.07d*E; Max = 2420870 + 325.33d*E (JD2420500 -
             24700); since JD2424700 - see Table.
X     Oph    VBA (A = 0.34", Porb = 485.3 yr; B - 9m, K1III, 0.4",
             142deg, 1980).
             The range of the combined brightness is given.
             P var. Max = 2416416 + 336.61d*E (JD2416400 - 26000);
             Max = 2426161 + 331.28d*E (JD2426000 - 32500); Max =
             2432788 + 335.50d*E (JD2432500 - 38000);
             since JD2438000 - see Table.
Y     Oph    SB1? Porb = 2612d? P var. Before JD2427000
             Max = 2408694.77 + 17.11884d*E; since
             JD2432000 - see Table. [A/H] = -0.2.
Z     Oph    P var. Max = 2411896 + 349.0d*E (JD2411800 - 21000)
             [00458]; Max = 2420962 + 352.1d*E (JD2421000 - 25000);
             Max = 2425183 + 347.4d*E (JD2425000 - 31000);
             Mean elements after JD2431000 - see Table.
RR    Oph    P var. Nonlinear term: -0.009282d*E2.
RS    Oph    Previous outbursts: 1898, 1933, 1958.
             According to [07575], in 1972 - 1973 there were semiregular
             variations (Delta(m) ~0.5M, P = 50D - 70D).
RT    Oph    P var. Before JD2426500 Max = 2417452 +
             429.00d*E; Max = 2426461 + 422.67d*E (JD2426500 -
             34000); since JD2434500 - see Table. OH, H2O maser.
RU    Oph    P var. Before JD2422000 Max = 2417388 +
             200.95d*E; Max = 2422011 + 203.62d*E (JD2422000 -
             27300); Max = 2427298 + 200.5d*E (JD2427300 - 29000);
             Max = 2429305 + 203.88d*E (JD2429000 - 33000);
             during JD2433000 - 40500 - see Table.
RV    Oph    d = 0.015P; Min II 9.56, DII = 0.09P. The light curve
             share var.
RW    Oph    P var. Max = 242494 + 247.86d*E (JD2425000 - 34000).
             The Table gives mean elements.
RX    Oph    OH, H2O maser.
RY    Oph    P var. Max = 2415235 + 151.05d*E (JD2414700 - 24000);
             Max = 2424152 + 149.69d*E (JD2424000 - 31000); Max =
             2431339 + 150.94d*E (JD2431000 - 40000);
             since JD2440000 - see Table.
RZ    Oph    d = 0.030P.
SS    Oph    P var. Before JD2432500 Max = 2417330 + 179.88d*E.
ST    Oph    (k - b)2 = 0.03.
SV    Oph    The elements are valid since JD2422000.
SW    Oph    VB A (B 12.0m vis, 2.4", 91deg, 1943). d = 0.02P. P var.
             Min = 2418880.528 + 2.445948d*E (JD2418880 - 26200)
             [00001]; Min = 2431235.216 + 2.446086d*E (JD2427900 -
             33500) [02389]; since JD2434000 - see Table.
SX    Oph    d = 0.03P.
SZ    Oph    P var. Before JD2428400 Min = 2421057.556 + 3.708454d*E;
             since JD2442000 - see Table.
TT    Oph    [Fe/H] = -0.5.
TW    Oph    P2 = 2000d:. Associated with a nebula of variable
             brightness [03479].
UU    Oph    d = 0.024P. P var?
UX    Oph    P var. Max = 2426041 + 117.34d (JD2406430 - 28040);
             since JD2433100 - see Table.
VW    Oph    P var. Mean elements are given. During JD2422500 - 30600
             Max = 2430554 + 282.69d*E.
WW    Oph    Epoch of Min is given. The chart in [06286] is wrong.
WZ    Oph    Min II 9.82.
XX    Oph    A symbiotic object featuring deep fadings
             of long duration [09489].
AH    Oph    H2O maser.
AQ    Oph    The chart in [06286] is wrong.
BE    Oph    The data in [00278] refer to another star.
BF    Oph    SB? P var? since JD2430000 - see Table.
BN    Oph    80d <= P <= 250d.
DM    Oph    P var. P = 220d (1893 - 1910), P = 216d (1914 - 1928).
DQ    Oph    P = 35d is possible.
FK    Oph    V2 (NGC 6273).
GM    Oph    V12 (NGC 6284).
GR    Oph    P var. Max = 2415425 + 136d*E (1893 - 1908);
             during 1910 - 1928 - see Table.
IL    Oph    P2 = 140d:.
IW    Oph    In the field of the globular cluster NGC 6293,
             possible cluster member.
KM    Oph    In the field of the globular cluster NGC 6304, field star.
KO    Oph    In a dark nebula.
KQ    Oph    P2 = 1500d.
KR    Oph    P2 > 5000d.
OU    Oph    V70 (NGC 6266).
PU    Oph    VB (A = V29 (NGC 6266), the data are in the Table; B = V28
             (NGC 6266), 16.6m - 17m, 4B, 4.8", 7deg), B: RRAB,
             Max = 2433423.52 + 0.49749d*E, M - m = 0.15P.
V0378 Oph    Min II 14.2. In the region of the open cluster CR 359.
             Epoch of Max is given.
V0380 Oph    Porb = 0.16d. Blue.
V0391 Oph    In the region of the open cluster CR 359. P var?
             Before JD2427000 Min = 2425501.425 + 2.89558d*E [00432];
             since JD2441500 - see Table.
V0392 Oph    Red.
V0402 Oph    P var. Max = 2425364 + 154d*E (JD2425350 - 670);
             since JD2425670 - see Table.
V0413 Oph    Delta(S) = 3. Blazhko effect?
V0414 Oph    B - V: +0.41, +0.77.
V0423 Oph    In the region of the open cluster CR 359.
V0426 Oph    Outbursts separated by 17d - 55d [08079]; in 1976 - 77 the
             cycle was 32.3d. Outside outbursts 12.7m - 13.3m, waves
             with a cycle of 20 - 30 Min and slower variations.
V0438 Oph    H20 Maser.
V0439 Oph    B - V: +0.63, +0.97.
V0442 Oph    Porb = 0.14056d.
V0445 Oph    VB A (B 13.04m y, 21"nf). (k - b)2 = 0.35; Delta(S) = 2.
             According to [05692], Blazhko effect (Pi > 2000d).
V0449 Oph    P var. Before JD243900 Min = 2428696.465 +
             1.243078d*E; Min = 2442959.607 + 1.243095d*E
             (JD2439000 - 43000); since JD2443000 - see Table.
V0451 Oph    Min II 8.31; Min II - Min I = 0.494P; DII = 0.12P.
V0452 Oph    Delta(S) = 5:.
V0455 Oph    P var? The Table gives mean elements which need
             confirmation.
V0456 Oph    Min II 10.5. P var. Before JD2436100 Min =
             2428422.341 + 1.015986d*E [00476]; since JD2441800 - see
             Table.
V0465 Oph    B - V: +0.68, +1.10. P var?
V0471 Oph    Very red.
V0478 Oph    B - V: +0.86, +1.33. [A/H] = -0.7.
             The elements need confirmation.
V0487 Oph    D <= 0.14P. In the region of the open cluster Cr 359.
V0496 Oph    In the region of the open cluster Cr 359.
V0501 Oph    Min II 11.1.
V0502 Oph    Min II 8.81. P var. Since JD2434500 - see Table.
V0506 Oph    Min II 12.0. In the region of the open cluster Cr 359.
V0508 Oph    Min II 10.59.
V0509 Oph    In the region of the open cluster Cr 359.
V0511 Oph    Min II 13.7. In the region of the open cluster Cr 359.
V0515 Oph    Max = 2425600 + 300d*E (JD2425600 - 26700); P = 140d
             (JD2426700 - 27300); during JD2427300 - 30200 - see Table.
V0516 Oph    In the region of the globular cluster NGC 6304.
V0517 Oph    In the region of the globular cluster NGC 6304.
V0521 Oph    P = 164d (JD2415000 - 24600); P2 - 4000d.
V0526 Oph    Min II 13.6.
V0527 Oph    Min II 14.8.
V0532 Oph    P >= 6000d.
V0533 Oph    P >= 80d.
V0534 Oph    d = 0.03P.
V0535 Oph    d = 0.025P.
V0536 Oph    d = 0.04P:.
V0537 Oph    Min II 12.8.
V0540 Oph    d = 0.05P; Min II 13.4.
V0541 Oph    [A/H] = -1.0. In the region of the globular cluster
             NGC 6401; cluster non-member?
V0543 Oph    Min II 13.6.
V0549 Oph    Min II 14.0.
V0550 Oph    Min II 13.0.
V0554 Oph    [A/H] = -1.1.
V0555 Oph    Sharp and flat maxima. Blazhko effect?
V0557 Oph    Min II 15.7. In the region of the open cluster Cr 359.
V0558 Oph    B - V: +0.57, +0.68. [Fe/H] = -1.48. According to [09037],
             P = 0.299d.
V0564 Oph    [Fe/H] = -1.37. Epoch of Min is given. P var. Nonlinear
             term: +0.0073d*(E + 10)**2.
V0565 Oph    P = 0.3957d is possible. Photoelectric observations of
             1968 contradict the elements [05746].
V0566 Oph    dI = 0.048P; Min II 7.89, dII = 0.06P. P var. Before
             JD2440500 Min = 2436744.4200 + 0.40964091d*E [08287]; since
             JD2440500 - see Table.
V0567 Oph    (k - b)2 = 0.22; Delta(S) = 0. According to [07984],
             Max = 2441134.467 + 0.1300729d*E.
V0568 Oph    Red.
V0570 Oph    VB A (B 16.3m, 5", 90deg).
V0572 Oph    In the region of the open cluster Cr 359.
V0573 Oph    d = 0.034P. In the region of the open cluster Cr 359.
V0574 Oph    P2 ~500d.
V0577 Oph    Min II 11.9. Min II - Min I = 0.583P. DII = 0.050P.
             e = 0.22.
V0580 Oph    VB A (B 15.5m, 0.2').
V0585 Oph    A long-period variation is superimposed?
V0586 Oph    In the region of the open cluster Cr 359.
V0590 Oph    Min II 13.6.
V0592 Oph    Max = 2427227 + 78d*E (JD2426100 - 29400);
             during JD2429400 - 30150 - see Table.
             After intervals of irregular variability the periodicity
             resumes without phase shift.
V0605 Oph    Epoch of Min is given.
V0618 Oph    Min II 14.7:.
V0636 Oph    d = 0.030P.
V0683 Oph    P var. The light curve shape varies.
V0687 Oph    P may be twice longer.
V0693 Oph    Blazhko effect? [05692].
V0695 Oph    P var? The light curve shape varies.
V0698 Oph    P var? since JD2442950 - see Table.
V0700 Oph    B - V: +0.49, +0.50. [Fe/H] = -2.10.
V0716 Oph    Delta(S) = 7.
V0720 Oph    VI (NGC 6171). Cluster non-member.
V0722 Oph    P var. Max = 2437089.456 + 0.6190385d (JD2419900 - 37100)
             [07806]; since JD2436700 - see Table.
V0729 Oph    P var. Max = 2437492.766 + 0.4685794d*E (JD2423500 - 37800)
             [03560]; since JD2437400 - see Table.
V0732 Oph    Unusual light curve (sharp Max; primary Min; broad Max;
             secondary Min 15.2).
V0734 Oph    P var. Max = 2420636.497 + 0.562489d*E (JD2420600 -
             29100); during JD2429100 - 37150 - see Table.
V0735 Oph    Min II 10.6.
V0737 Oph    P = 374d is possible.
V0767 Oph    According to [00104], waves with Delta(m) = 0.3m - 1.4m vis
             of 50d - 110d duration; mean brightness var,
             Delta(m) ~0.4m in 800d - 1000d.
V0782 Oph    Very red.
V0784 Oph    B - V: +0.26, +0.56. The period should be checked.
V0786 Oph    Red.
V0788 Oph    Blazhko effect? Pi = 115d.
V0799 Oph    P = 215d is possible.
V0802 Oph    Red.
V0816 Oph    B - V: +0.25, +0.63.
V0822 Oph    Blazhko effect?
V0823 Oph    In the region of the open cluster IC 4665.
V0825 Oph    In the region of the open cluster IC 4665.
V0829 Oph    Blazhko effect? Pi = 165d.
V0832 Oph    Red.
V0838 Oph    P2 ~500d is possible.
V0839 Oph    mu = 0.041", ro = 292deg. Min II 9.38.
V0840 Oph    VB A (B 12m, 16", 116deg).
V0841 Oph    Max = 2396146.
V0843 Oph    SN Kepler. Max 2307193. Gaseous remnant.
V0844 Oph    Min II 14.9.
V0845 Oph    VB A (B 15.7m).
V0847 Oph    Min II 13.1.
V0848 Oph    Min II 13.4.
V0851 Oph    Max = 2425828 + 95d*E (JD2425600 - 29700);
             during JD2429700 - 34250 - see Table.
V0854 Oph    According to [08116], the spectrum
             resembles that of a T Tau - type star.
V0868 Oph    Min II 13.6. In the region of the open cluster Cr 359.
V0870 Oph    In the region of the open cluster Cr 359.
V0872 Oph    P = 0.825d is possible.
V0878 Oph    Min II 16.5. In the region of the open cluster Cr 359.
V0911 Oph    P2 = 81d, P3 = 114d. P4 > P3? Standstills up to 100d.
V0919 Oph    VB A (B sp).
V0920 Oph    Min II 15.9.
V0924 Oph    Min II 16.4.
V0929 Oph    d = 0.050P.
V0934 Oph    E type is possible.
V0936 Oph    In the region of the open cluster Cr 359.
V0938 Oph    Min II 15.3. In the region of the open cluster Cr 359.
V0940 Oph    Min II 15.6.
V0941 Oph    Min II 16.5.
V0943 Oph    Min II 16.4. In the region of the open cluster Cr 359.
V0945 Oph    Min II 15.1. In the region of the open cluster Cr 359.
V0947 Oph    Min II 14.5. In the region of the open cluster Cr 359.
V0952 Oph    P = 0.954d is possible.
V0954 Oph    In the region of the open cluster Cr 359. Min II 14.9.
             According to [03500], const, V = 12.86m, B - V = +1.36m,
V0959 Oph    P var? Max = 2429785.419 + 0.084857d*E
             (JD2429785 - 845) [02757]; during JD2443719 - 732 - see
             Table; other possible elemente:
             Max = 2443726.469 + 0.07786d*E.
V0960 Oph    In the region of the open cluster Cr 359.
V0963 Oph    Min II 15.1. In the region of the open cluster Cr 359.
V0968 Oph    [Fe/H] = -1.48. In the region of the open cluster Cr 359.
V0969 Oph    Min II 13.8:. In the region of the open cluster Cr 359.
V0977 Oph    In the region of the globular cluster NGC 6426.
V0978 Oph    In the region of the globular cluster NGC 6426.
V0979 Oph    V11 (NGC 6426). Cluster non-member.
V0980 Oph    In the the region of globular cluster NGC 6426.
             P = 0.25740d is possible.
V0983 Oph    In the region of the open cluster Cr 359.
V0986 Oph    In July 1980 Vr varied with P = 0.179d, 0.147d, 0.225d,
             and possibly 0.097d, but there were no spectrum variations,
             and the photometric P = 0.323d was not noticeable in Vr.
             SB? Porb = 15d - 20d; there is also excess power
             at low frequences in the photometric data. Earlier
             studies revealed photometric periods 0.284d - 0.4d
             and violation of periodicity.
V0987 Oph    d = 0.02P. Min II 14.6. In the region of the open cluster
             Cr 359.
V0998 Oph    In the region of the globular cluster NGC 6171.
V0999 Oph    In the region of the globular cluster NGC 6171.
V1000 Oph    Blazhko effect?
V1002 Oph    Min II 15.2.
             RRC type with twice shorter P is possible.
V1004 Oph    Blazhko effect?
V1010 Oph    Min II 6.46. P var. P = 0.661464d (JD2415000 - 25000)
             [05738]; since JD2425000 - see Table, nonlinear term:
             -3.87d*10**(-10)*E**2. Min I var.The light curve shape and
             the depth of Min I var.
V1011 Oph    Blazhko effect?
V1015 Oph    D <= 0.23P, d < 0.02P; Min II 14.5.
V1017 Oph    [Fe/H] = -1.25. P var? Max = 2437433.935 + 0.2343d*E
             (JD2437433 - 514) [03625]. During
             JD2442954 - 45140 - see Table.
             According to [09037], P = 0.361d.
V1018 Oph    Possibly eclipsing.
V1021 Oph    Delta(m) var. B - V: +0.42, +0.62.
V1022 Oph    d = 0.06P:; Min II 15.95.
V1024 Oph    Max = 2437433.559 + 0.5914d*E (JD2437433 - 514)
             [03625]. During JD2442954 - 45140 - see Table.
             RR(B) type is possible; P = 0.371d satisfies the
             observations during JD2442954 - 44407.
V1026 Oph    Max = 2437433.562 + 0.6563d*E (JD2437433 - 514)
             [03625]. During JD2442954 - 45140 - see Table.
V1028 Oph    Blazhko effect?
V1032 Oph    P > 1.0d is not excluded.
V1033 Oph    Max = 2437433.714 + 0.4845d*E (JD2437433 - 514)
             [03625]. During JD2442954 - 45140 - see Table.
V1035 Oph    Max = 2437433.388 + 0.6100d*E (JD2437433 - 514)
             [03625]; during JD2442954 - 45140 - see Table.
V1039 Oph    P = 0.3166d is possible.
V1040 Oph    The light curve shape var.
V1041 Oph    [Fe/H] = -1.06.
V1042 Oph    The light curve shape var. Max = 2437433.633 + 0.5528d
             (JD2437433 - 514) [03625]. During JD2442954 - 45140 - see
             Table.
V1052 Oph    Max = 2437433.537 + 0.7546d*E (JD2437433 - 514)
             [03625]; during JD2442954 - 45140 - see Table.
V1054 Oph    VB Wolf 630AB (A 9.76m V, 12.47mu; B 9.78m V; A = 0.22",
             Porb = 1.71665 yr; C = Wolf 629, 11.70m V,14.75mu,
             dM4, 72", D = vB8, 16.7m V, 221", common mu). mu = 1.19",
             ro = 222deg. Lx/Lopt(V) = 0.05.
V1072 Oph    P var. Max = 2439025.31 + 0.444715d*E (JD2438500 - 39025);
             since JD2442800 - see Table.
V1075 Oph    Red.
V1077 Oph    P var. Max = 2438614.40 + 0.373926d*E (JD2438200 - 700);
             Max = 2442871.516 + 0.37384d*E (JD2442810 - 910):
             Max = 2442983.345 + 0.373911d*E (JD2442920 - 3330);
             since JD2443330 - see Table.
V1089 Oph    VB AB (B 16.4m, 2", 45deg).
V1099 Oph    Red.
V1100 Oph    Red.
V1111 Oph    OH, H2O, SiO maser.
V1120 Oph    Min II 14.3.
V1121 Oph    Soft X-ray source.
V1135 Oph    [Ca/H] = -0.74.
V1141 Oph    P var? The light curve shape var?
V1142 Oph    P var? The light curve shape var?
V1146 Oph    P = 185.2d is possible.
V1153 Oph    P = 153.0d is possible.
V1157 Oph    B - V: +0.42, +0.66.
V1161 Oph    P = 0.49d is possible [06438].
V1168 Oph    P var? The light curve shape var?
V1170 Oph    P = 360d: is possible [06438].
V1174 Oph    P var? The light curve shape var?
V1176 Oph    P = 269.0d is possible.
V1179 Oph    P var? The light curve shape var?
V1185 Oph    Other possible elements: Max = 2435630 + 177d*E [00001].
V1195 Oph    One more Max 2435637 (1956). Type M is possible.
V1203 Oph    P = 315d is possible [06438].
V1204 Oph    P = 144d: or P = 191d: are possible.
V1235 Oph    UV type is possible.
V1240 Oph    P = 0.42136d is possible.
V1244 Oph    The light curve shape var?
V1258 Oph    P var?
V1261 Oph    The light curve is not typical for the P in the Table [06438].
V1262 Oph    The light curve is not typical for the P in the Table [06438].
V1276 Oph    [Ca/H] = -0.1.
V1296 Oph    [Ca/H] = -0.9.
V1299 Oph    The light curve shape var?
V1300 Oph    P = 235d: is possible.
V1305 Oph    Min II 17.9:.
V1307 Oph    The light curve shape var? Spurious period? [06438].
V1323 Oph    P var?
V1332 Oph    [Ca/H] = -0.64.
V1348 Oph    The light curve shape var?
V1355 Oph    The light curve shape var?
V1403 Oph    P = 215d?
V1423 Oph    The light curve shape var?
V1426 Oph    P var?
V1451 Oph    P = 179.4d?
V1474 Oph    P = 127d:?
V1491 Oph    P = 328.0d?
V1492 Oph    The light curve shape var?
V1505 Oph    P = 86d:?
V1512 Oph    The light curve shape var?
V1526 Oph    P = 0.29745d?
V1532 Oph    P = 144.4d?
V1534 Oph    P = 198.8d?
V1548 Oph    The minor planet (336) Lacadiera.
V1554 Oph    P = 136.0d?
V1568 Oph    P = 275.5d?
V1571 Oph    P var?
V1573 Oph    Type E?
V1583 Oph    P - spurious?
V1616 Oph    Type E?
V1628 Oph    The light curve shape var?
V1637 Oph    [Ca/H] = -0.44.
V1661 Oph    The light curve shape var?
V1666 Oph    P = 154.2d?
V1676 Oph    Close optical companion?
V1682 Oph    P = 118.0d?
V1687 Oph    Type CW?
V1702 Oph    P = 121d?
V1705 Oph    P var?
V1710 Oph    P = 0.37422d?
V1731 Oph    The light curve shape var?
V1736 Oph    P = 143.8d?, P = 244.5d?
V1744 Oph    P = 191.6d?
V1748 Oph    A var. Type CW?
V1754 Oph    P = 128.4d?
V1768 Oph    The light curve shape var?
V1775 Oph    Type EW?
V1793 Oph    P = 170d:?
V1803 Oph    The star is not SVS 438.
V1805 Oph    The light curve shape var?
V1811 Oph    Min II 17.9:.
V1814 Oph    P = 160.4d?
V1822 Oph    P var?
V1829 Oph    P = 143.2d?
V1840 Oph    V 12 (NGC 6333 = M9). Cluster member.
V1841 Oph    The light curve shape var?
V1845 Oph    V7 (NGC 6333 = M9). Cluster member.
V1853 Oph    The light curve shape var?
V1860 Oph    [Ca/H] = -0.49.
V1861 Oph    P = 142.0d?
V1864 Oph    V3 (NGC 6333 = M9). Cluster member.
V1886 Oph    The light curve shape var?
V1889 Oph    P = 316.0d?
V1895 Oph    The light curve shape var?
V1905 Oph    P = 149.0d?
V1919 Oph    P = 102.8d?, P = 227.0d?
V1939 Oph    P = 330.0d?
V1946 Oph    The light curve shape var?
V1952 Oph    P = 248.0d?
V1953 Oph    P = 199d:?, P = 235d:?
V1954 Oph    P = 159.6d?
V1973 Oph    P = 0.24154d?
V1989 Oph    A var?
V1990 Oph    P = 121d:?
V1991 Oph    The light curve shape var?
V1994 Oph    P = 170.0d?
V1998 Oph    P = 270.5d?
V2002 Oph    The light curve shape var?
V2003 Oph    [Ca/H] = -0.96.
V2009 Oph    V5 (NGC 6356). Cluster member.
V2010 Oph    [CA/H] = -0.79.
V2016 Oph    [CA/H] = -0.96.
V2042 Oph    P var. Max = 2430146.478 + 0.5385d*E (JD2429100 -
             30202); since JD2436700 - see Table.
V2045 Oph    The chart in [05159] is wrong.
V2048 Oph    SB2 [06598]. In the region of the open cluster Cr 359.
             Along with irregular light variations typical for be stars
             there are rapid flares with the amplitudes up to 1.8m
             (lambda eff = 5800 A) [06150]. It is not excluded that the
             flares occur on a fainter companion of the system.
V2051 Oph    Usually - 15.0m with strong flickering of brightness
             (up to 0.4m is 5 minutes) and rare flares. At the same
             time the eclipses are observed with depth to 2.5m with the
             elements: Min = 2444787.32124 + 0.062427865d*E [09550];
             D = 0.0088P:, d = 0.0065P.
V2058 Oph    In the dark nebula in the rho Oph region.
V2059 Oph    In the dark nebula in the rho Oph region.
V2061 Oph    In the region of the globular cluster NGC 6171 (M 107).
V2062 Oph    In the dark nebula in the rho Oph region.
V2063 Oph    The minor planet (64) Angelina.
V2064 Oph    In the dark nebula in the rho Oph region.
V2101 Oph    In a dark nebula.
V2102 Oph    In the region of the globular cluster NGC 6293.
V2105 Oph    Vr = 100 km/s.
V2106 Oph    <Vr> = -102 km/s.
V2108 Oph    H2O, SiO maser.
V2112 Oph    The primary oscillation with A1 = 0.0172m
             (see Table) is superimposed by the secondary one
             (A2 = 0.0061m) with the elements:
             Max = 2444114.531: + 0.1449461d*E.
V2116 Oph    X-ray pulsar. The pulse period is decreasing: 135s (1971),
             112.076s (1979), 109.668s (1980) [09553]. The spin-period
             may be twice longer.
V2118 Oph    Probably rapidly rotating single spotted F type star.
             Max brightness epoch is given.
V2119 Oph    In the region of the globular cluster
             NGC 6284. Not a member of the cluster.
V2120 Oph    V6 (NGC 6284). In the region of the globular cluster
             NGC 6284. Not a member of the cluster.
V2121 Oph    V10 (NGC 6284). In the region of the globular cluster
             NGC 6284. Not a member of the cluster.
V2122 Oph    In the region of the globular cluster NGC 6284. Not
             a member of the cluster.
V2123 Oph    V11 (NGC 6284). In the region of the globular cluster
             NGC 6284. Not a member of the cluster.
V2124 Oph    In the region of the globular cluster NGC 6284. Not
             a member of the cluster.
V2391 Oph    Porb = 88.13yr. Component B is a suspected variable star
             (NSV 24260) and may be the cause of variations.
V2561 Oph    Not a supernova.
tet   Oph    SB1 (Porb = 11.44d [06597]).
             The basic oscillation (see Table) is superimposed by
             oscillations with the periods: P1 = 0.092551d,
             P2 = 0.069452d, P3 = 0.0555d, P4 = 0.0464d, P02 =
             0.137255d, P13 = 0.13845d, P24 = 0.13990d, P03 = 0.09185d.
khi   Oph    SB 1 (Porb = 138.8d [09558]).
ome   Oph    P = 1.5d?
R     Ori    SC 5/9.5 E. P var. Max = 2399420 + 378d*E
             (JD2395600 - 99500); Max = 2412687 + 378.1d*E
             (JD2403200 - 12700); Max = 2414230 + 366.5d*E
             (JD2413800 - 16800); Max = 2417943 + 378.1d*E
             (JD2416800 - 21350); Max = 2421352 + 384.9d*E
             (JD2421350 - 24100); since JD2424100 - see Table.
S     Ori    VB A (B 10.9m, 47", 228deg). SiO maser. P var.
             Max = 2404538 + 412.00d*E (JD2404520 - 13600);
             Max = 2414014 + 427.15d*E (JD2414000 - 19150);
             Max = 2419567 + 416.11d*E (JD2419570 - 22890);
             Max = 2423312 + 407.10d*E (JD2423320 - 31050);
             Max = 2431454 + 438.53d*E (JD2431500 - 39000)
             [03765]; since JD2439000 - see Table.
T     Ori    In the T-association of the Orion nebula. Connected with
             a cometary nebula.
U     Ori    SiO, OH, H2O maser. P var. Max = 2409881 + 374.5d*E
             (JD2409800 - 15900); Max = 2415871 + 367.9d*E
             (JD2415900 - 21000); Max = 2421016 + 376.0d*E
             (JD2421000 - 29300); Max = 2428164 + 368.3d*E
             (JD2428100 - 32900) [00960];
             Max = 2433336 + 372.7d*E (JD2432900 - 43800);
             since JD2443800 - see Table.
V     Ori    P var. Max = 2413656 + 264.8d*E (JD2411800 - 18700);
             Max = 2418987 + 271.7d*E (JD2418700 - 24600);
             Max = 2424695 + 263.7d*E (JD2424600 - 29400)
             [00960]; Max = 2430769 + 269.9d*E (JD2430700 - 36200);
             since JD2437700 - see Table.
W     Ori    Mean magnitude varies with P = 2450d.
Z     Ori    Min II 9.9; d = 0.013P.
RS    Ori    P var. Max = 2428073.205 + 7.566836d*E (JD2416500 -
             33000); since JD2435000 - see Table.
RT    Ori    Mean magnitude varies with P = 3200d.
RU    Ori    In the region of the nebula IC 434.
RV    Ori    In the region of the nebula IC 434.
RW    Ori    In the region of the nebula IC 434.
RX    Ori    In the region of the Orion nebula T-association.
RZ    Ori    In the region of the Orion nebula T-association.
SS    Ori    In the region of the Orion nebula T-association.
ST    Ori    In the region of the Orion nebula T-association.
SU    Ori    In the region of the Orion nebula T-association.
SV    Ori    In the region of the Orion nebula T-association.
SW    Ori    In the region of the Orion nebula T-association.
SX    Ori    In the region of the Orion nebula T-association.
SY    Ori    In the region of the Orion nebula T-association.
SZ    Ori    In the region of the Orion nebula T-association.
TT    Ori    In the region of the Orion nebula T-association.
TU    Ori    In the region of the Orion nebula T-association.
TV    Ori    In the region of the Orion nebula T-association.
TW    Ori    In the region of the Orion nebula T-association.
TX    Ori    VB A (B = TY Ori, 42.4", 45deg); in the region of
             the nebula IC 434.
TY    Ori    VB B (A = TX Ori); in the region of the nebula IC 434.
TZ    Ori    In the region of the nebula IC 434.
UW    Ori    Min II 11.6.
UY    Ori    In the region of the Orion nebula T-association.
UZ    Ori    In the region of the Orion nebula T-association.
VV    Ori    Min II 5.50; dI = 0.055P; dII = 0.064P.
             There is third component in the system
             (Porb = 119.09d [08045]).
VW    Ori    In the region of the Orion nebula T-association.
VX    Ori    In the region of the Orion nebula T-association.
VY    Ori    VB A (B = 16.6mV, 16", 135deg). In the region of the Orion
             nebula T-association.
VZ    Ori    In the region of the Orion nebula T-association.
WW    Ori    In the region of the Orion nebula T-association.
WX    Ori    VB A (B 17m, 11", 10deg). In the region of the Orion nebula
             T-association.
WY    Ori    In the region of the Orion nebula T-association.
WZ    Ori    In the region of the Orion nebula T-association.
XX    Ori    In the region of the Orion nebula T-association.
XY    Ori    In the region of the Orion nebula T-association.
XZ    Ori    The periodicity in light variations is possible.
             In the region of the Orion nebula T-association.
YY    Ori    Emission. In the region of the Orion nebula T-association.
YZ    Ori    In the region of the Orion nebula T-association.
ZZ    Ori    In the region of the Orion nebula T-association.
AA    Ori    In the region of the Orion nebula T-association.
AB    Ori    In the region of the Orion nebula T-association.
AC    Ori    In the region of the Orion nebula T-association.
AE    Ori    In the region of the Orion nebula T-association.
AF    Ori    In the region of the Orion nebula T-association.
AG    Ori    VB A (B 16.4mV, 16", 185deg). In the region of the Orion
             nebula T-association.
AH    Ori    In the region of the Orion nebula T-association.
AI    Ori    In the region of the Orion nebula T-association.
AK    Ori    In the region of the Orion nebula T-association.
AL    Ori    In the region of the Orion nebula T-association.
AM    Ori    VB A (B 20.3mV, 3.5", 320deg). In the region of the Orion
             nebula T-association.
AN    Ori    In the region of the Orion nebula T-association.
AO    Ori    In the region of the Orion nebula T-association.
AP    Ori    In the region of the Orion nebula T-association.
AQ    Ori    In the region of the Orion nebula T-association.
AR    Ori    VB A (B 2", 240deg). In the region of the Orion nebula
             T-association.
AS    Ori    In the region of the Orion nebula T-association.
AT    Ori    In the region of the Orion nebula T-association.
AU    Ori    In the region of the Orion nebula T-association.
AV    Ori    VB A (B 18.7mV, 6", 305deg). In the region of the nebula
             T-association.
AW    Ori    In the region of the Orion nebula T-association.
AX    Ori    In the region of the Orion nebula T-association.
AY    Ori    In the region of the Orion nebula T-association.
AZ    Ori    In the region of the Orion nebula T-association.
BB    Ori    In the region of the Orion nebula T-association.
BC    Ori    In the region of the Orion nebula T-association.
BD    Ori    In the region of the Orion nebula T-association.
BE    Ori    In the region of the Orion nebula T-association.
BF    Ori    In the region of the Orion nebula T-association.
BG    Ori    In the region of the nebula IC 434.
BH    Ori    In the region of the Orion nebula T-association.
BK    Ori    P var. Max = 2422016 + 338.0d*E (JD2413550 - 22100);
             Max = 2428880 + 326.5d*E (JD2422300 - 28880);
             Max = 2429940 + 345.3d*E (JD2428880 - 29940);
             Max = 2432892 + 327.7d*E (JD2429940 - 32900);
             Max = 2438800 + 346.3d*E (JD2432900 - 38800);
             since JD2438800 - see Table.
BM    Ori    In the region of the Orion nebula T-association. In the
             cluster NGC 1976. Orion Trapezium
             member: teta**1 Ori B (A = V1016 Ori; B 8.7", 32deg;
             C 5.13m, 13.1", 131deg; D 6.70m, 21.6", 96deg). d = 0.05P;
             Min II 7.98. Shape of the light curve and depths of minima
             vary.
BO    Ori    In the region of the Orion nebula T-association.
BP    Ori    In the region of the Orion nebula T-association.
BS    Ori    In the region of the Orion nebula T-association.
BT    Ori    In the region of the Orion nebula T-association.
BU    Ori    In the region of the Orion nebula T-association.
BV    Ori    In the region of the Orion nebula T-association.
BW    Ori    In the region of the Orion nebula T-association.
BX    Ori    In the region of the Orion nebula T-association.
BY    Ori    In the region of the Orion nebula T-association.
BZ    Ori    In the region of the Orion nebula T-association.
CC    Ori    In the region of the Orion nebula T-association.
CD    Ori    In the region of the Orion nebula T-association.
CE    Ori    In the region of the Orion nebula T-association.
CF    Ori    In the region of the Orion nebula T-association.
CG    Ori    In the region of the Orion nebula T-association.
CH    Ori    In the region of the Orion nebula T-association.
CI    Ori    VB A (B 9.70m, 12.9", 88deg).
CM    Ori    P var?
CN    Ori    Porb = 0.163097d.
             Light curve is superposed by oscillations with
             the following elements: Max0 = 2444941.5032 +
             0.163097d*E (A0 = 0.2m), Max1 = 2444941.573 +
             0.15946d*E (A1 = 0.1m) [09471].
             Sometimes smaller rapid light oscillations are also
             observed with periods 24.3s - 29.5s (A<1%).
CO    Ori    Member of the T-association
             CO Ori. VB A (B 13m, 1", 280deg).
CP    Ori    Min II 11.2. P var [02545].
CT    Ori    SRD? P = 68d? [09496].
CW    Ori    Min II 13.2.
DK    Ori    In the region of the Orion nebula T-association.
             VB (ro < 3").
DL    Ori    In the region of the Orion nebula T-association.
DM    Ori    In the region of the Orion nebula T-association.
DN    Ori    Min II 9.9; d = 0.026P. P var. Min I = 2428497.51 +
             12.9649d*E (JD2425200 - 28600); since
             JD2435570 - see Table.
DY    Ori    B - V: +0.58, +1.72.
EG    Ori    d = 0.086P. P var?
EQ    Ori    Min II 10.3. P var. Min I = 2425889.706 + 1.74608d*E
             (JD2425600 - 26700) [02839]; Min I = 2429219.467 +
             1.74611d*E (JD2427700 - 31000) [00001];
             since JD2431000 - see Table.
ER    Ori    VB A (B 13.6", 0deg). Min II 9.97. P var. Min I =
             2426336.6485 + 0.4233955d*E (JD2426330 - 33920)
             [00279]; Min I = 2434765.6306 + 0.42340620d*E
             (JD2433920 - 35475) [02278]; Min I = 2436508.7851 +
             0.4234009d*E (JD2435475 - 40000) [03787];
             since JD2440000 - see Table. Shape of the light curve
             varies.
ET    Ori    Min II 11.3. P var?
EW    Ori    Min II 10.5; Min II - Min I = 0.529P.
             In the region of the open cluster CR 70.
             In [00007] Min II are accepted to be Min I, and vice
             versa (Min II - Min I = 0.47P).
             For decisive choice of the Min I epoch photoelectric
             observations are necessary. P var? Min II =
             2429974.810 + 6.9368005d*E [00007]; since
             JD2430000 - see Table.
EY    Ori    Min II 9.54; d = 0.003P. In the region of the Orion
             nebula T-association. P var.
             Min I = 2427310.420 + 16.787450d*E [00007];
             since JD2427500 - see Table.
EZ    Ori    In the region of the Orion nebula T-association.
FF    Ori    Min II 10.3.
FH    Ori    d = 0.035P. P var.
FI    Ori    VB A (B 10.5m, 5", 323deg).
             Shape of the light curve varies, probably periodically
             [03790, 05475].
FK    Ori    P var. Min = 2427773.390 + 1.947447d*E (JD2426900 -
             37500); since JD2437500 - see Table.
FL    Ori    P var. Min = 2427452.271 + 1.550971d*E (JD2427450 -
             29600) [03115]; Min = 2430400.649 + 1.55093d*E
             (JD2429600 - 30400);Min = 2432517.755 + 1.550991d*E
             (JD2430400 - 32900); Min = 2434459.571 + 1.550965d*E
             (JD2432900 - 35050); Min = 2436649.568 + 1.550995d*E
             (JD2435050 - 40600); since JD2440600 - see Table.
FO    Ori    Min II 9.7; d = 0.005P.
FR    Ori    Min II 11.1.
FT    Ori    Min II 9.60; DII = 0.08P; Min II - Min I = 0.73P. P var.
             Min I = 2433009.553 + 3.150404d*E (JD2426380 - 38000)
             [02758]; since JD2438000 - see Table.
             The period of apsidal motion 520 +- 100 years [07358].
FU    Ori    Member of FU Ori T-association. In the dark globule B35.
             Connected with a bright cometary nebula and the bright
             hydrogen nebula S 280. Light maximum was in summer
             1937. IN 1980 - 10.6m B.
FZ    Ori    Min II 11.2.
GG    Ori    Min II 11.1; Min II - Min I = 0.427P.
GP    Ori    SC 7/8- .
GQ    Ori    VB A (B 9.7m, 31", 324deg).
GW    Ori    In the T-association CO Ori.
GX    Ori    In the T-association CO - Ori.
GY    Ori    In the T-association CO - Ori.
GZ    Ori    In the region of the Orion nebula T-association.
HH    Ori    In the region of the Orion nebula T-association.
HI    Ori    In the T-association CO - Ori.
HK    Ori    In the T-association CO - Ori.
             Connected with a bright cometary nebula. CO, CH, OH
             emission.
HL    Ori    In the region of the Orion nebula T-association.
HM    Ori    In the T-association CO - Ori.
HN    Ori    In the region of the Orion nebula T-association.
HO    Ori    In the region of the Orion nebula T-association.
HP    Ori    In the region of the Orion nebula T-association.
HQ    Ori    In the region of the Orion nebula T-association.
HR    Ori    In the region of the Orion nebula T-association.
HS    Ori    In the region of the Orion nebula T-association.
HT    Ori    In the region of the Orion nebula T-association.
HU    Ori    In the region of the Orion nebula T-association.
HV    Ori    In the region of the Orion nebula T-association.
HW    Ori    In the region of the Orion nebula T-association.
HX    Ori    In the region of the Orion nebula T-association.
HY    Ori    In the region of the Orion nebula T-association.
HZ    Ori    In the region of the Orion nebula T-association.
II    Ori    In the region of the Orion nebula T-association.
IK    Ori    In the region of the Orion nebula T-association.
IL    Ori    In the region of the Orion nebula T-association.
IM    Ori    In the region of the Orion nebula T-association.
IN    Ori    In the region of the Orion nebula T-association.
IO    Ori    In the region of the Orion nebula T-association.
IP    Ori    In the region of the Orion nebula T-association.
IQ    Ori    In the region of the Orion nebula T-association.
IR    Ori    In the region of the Orion nebula T-association.
IS    Ori    In the region of the Orion nebula T-association.
IT    Ori    In the region of the Orion nebula T-association.
IU    Ori    In the region of the Orion nebula T-association.
IV    Ori    In the region of the Orion nebula T-association.
IW    Ori    In the region of the Orion nebula T-association.
IX    Ori    In the region of the Orion nebula T-association.
IY    Ori    In the region of the Orion nebula T-association.
IZ    Ori    In the region of the Orion nebula T-association.
KK    Ori    In the region of the Orion nebula T-association.
KL    Ori    In the region of the Orion nebula T-association.
KM    Ori    In the region of the Orion nebula T-association.
KN    Ori    In the region of the Orion nebula T-association.
KO    Ori    In the region of the Orion nebula T-association.
KP    Ori    In the region of the Orion nebula T-association.
KQ    Ori    In the region of the Orion nebula T-association.
KR    Ori    In the region of the Orion nebula T-association.
KS    Ori    In the region of the Orion nebula T-association.
KT    Ori    In the region of the Orion nebula T-association.
KU    Ori    In the region of the Orion nebula T-association.
KV    Ori    In the region of the Orion nebula T-association.
KW    Ori    In the region of the Orion nebula T-association.
KX    Ori    In the region of the Orion nebula T-association.
KY    Ori    In the region of the Orion nebula T-association.
KZ    Ori    In the region of the Orion nebula T-association.
LL    Ori    In the region of the Orion nebula T-association.
LM    Ori    In the region of the Orion nebula T-association.
LN    Ori    In the region of the Orion nebula T-association.
LO    Ori    In the region of the Orion nebula T-association.
LP    Ori    In the region of the Orion nebula T-association.
LQ    Ori    In the region of the Orion nebula T-association.
LR    Ori    In the region of the Orion nebula T-association.
LS    Ori    In the region of the Orion nebula T-association.
LT    Ori    In the region of the Orion nebula T-association.
LU    Ori    In the region of the Orion nebula T-association.
LV    Ori    In the region of the Orion nebula T-association.
LW    Ori    In the region of the Orion nebula T-association.
LX    Ori    In the region of the Orion nebula T-association.
LY    Ori    In the region of the Orion nebula T-association.
LZ    Ori    VB B (A 10.3m; B 14.1", 219deg). In the region of the
             Orion nebula T-association.
MM    Ori    In the region of the Orion nebula T-association.
MN    Ori    In the region of the Orion nebula T-association.
MO    Ori    In the region of the Orion nebula T-association.
MP    Ori    In the region of the Orion nebula T-association.
MQ    Ori    In the region of the Orion nebula T-association.
MR    Ori    In the region of the Orion nebula T-association.
MS    Ori    In the region of the Orion nebula T-association.
MT    Ori    In the region of the Orion nebula T-association.
MU    Ori    In the region of the Orion nebula T-association.
MV    Ori    In the region of the Orion nebula T-association.
MW    Ori    In the region of the Orion nebula T-association.
MX    Ori    In the region of the Orion nebula T-association.
MY    Ori    In the region of the Orion nebula T-association.
MZ    Ori    In the region of the Orion nebula T-association.
NN    Ori    In the region of the Orion nebula T-association.
NO    Ori    In the region of the Orion nebula T-association.
NP    Ori    In the region of the Orion nebula T-association.
NQ    Ori    In the region of the Orion nebula T-association.
NR    Ori    In the region of the Orion nebula T-association.
NS    Ori    In the region of the Orion nebula T-association.
NT    Ori    In the region of the Orion nebula T-association.
NU    Ori    In the region of the Orion nebula T-association. In the
             nebula NGC 1982. Dust shell.
NV    Ori    In the region of the Orion nebula T-association.
NW    Ori    In the region of the Orion nebula T-association.
NX    Ori    In the region of the Orion nebula T-association.
NY    Ori    VB B (A = V566 Ori; B 5", 135deg). In the region of the
             Orion nebula T-association.
NZ    Ori    In the region of the Orion nebula T-association.
OO    Ori    In the region of the Orion nebula T-association.
OP    Ori    In the region of the Orion nebula T-association.
OQ    Ori    In the region of the Orion nebula T-association.
OR    Ori    In the region of the Orion nebula T-association.
OT    Ori    In the region of the Orion nebula T-association.
OU    Ori    In the region of the Orion nebula T-association.
OV    Ori    In the region of the Orion nebula T-association.
OW    Ori    In the region of the Orion nebula T-association.
OX    Ori    In the region of the Orion nebula T-association.
OY    Ori    In the region of the Orion nebula T-association.
OZ    Ori    In the region of the Orion nebula T-association.
PP    Ori    In the region of the Orion nebula T-association.
PQ    Ori    In the region of the nebula IC 434.
PR    Ori    In the region of the Orion nebula T-association.
PS    Ori    In the region of the Orion nebula T-association.
PT    Ori    In the region of the Orion nebula T-association.
PU    Ori    In the region of the nebula IC 434.
PV    Ori    In the region of the Orion nebula T-association.
PW    Ori    In the region of the Orion nebula T-association.
PX    Ori    <Vr> =  + 298 km/s [09511]. In the region of the Orion
             nebula T-association.
PY    Ori    In the region of the Orion nebula T-association.
PZ    Ori    In the region of the Orion nebula T-association.
QQ    Ori    In the region of the Orion nebula T-association.
QR    Ori    In the region of T-association FU Ori.
QT    Ori    P var? Elements given in the Table are valid in the
             interval JD2429640 - 35550.
V0340 Ori    Epoch of Min brightness is given.
V0343 Ori    Min II 11.0. Shape of the light curve and depth of
             Min II vary.
V0347 Ori    In the region of the Orion nebula T-association.
V0348 Ori    In the region of the Orion nebula T-association.
V0349 Ori    In the region of the Orion nebula T-association.
V0353 Ori    In the region of the Orion nebula T-association.
V0354 Ori    In the region of the Orion nebula T-association.
V0355 Ori    In the region of the Orion nebula T-association.
V0356 Ori    In the region of the Orion nebula T-association.
V0357 Ori    In the region of the Orion nebula T-association.
V0358 Ori    In the region of the Orion nebula T-association.
V0359 Ori    In the region of the Orion nebula T-association.
             Epoch of Min HEI line intensity is given.
             According to [09512], P = 14.612d.
V0360 Ori    In the region of the Orion nebula T-association.
V0361 Ori    VB C (A 4.8m; B 6.1m, 52.4", 93deg; C 129", 97deg).
             In the region of the Orion nebula T-association.
V0362 Ori    In the region of the Orion nebula T-association.
V0363 Ori    In the region of the Orion nebula T-association.
V0364 Ori    In the region of the Orion nebula T-association.
V0365 Ori    In the region of the Orion nebula T-association.
V0366 Ori    In the region of the Orion nebula T-association.
V0367 Ori    In the region of the Orion nebula T-association.
V0368 Ori    In the region of the Orion nebula T-association.
V0369 Ori    In the region of the Orion nebula T-association.
V0370 Ori    In the T-association CO - Ori.
V0371 Ori    mu = 0.28", ro = 238deg.
V0372 Ori    In the region of the Orion nebula T-association.
V0373 Ori    In the region of the Orion nebula T-association.
V0374 Ori    In the region of the Orion nebula T-association.
V0375 Ori    In the region of the Orion nebula T-association.
V0376 Ori    In the region of the Orion nebula T-association.
V0377 Ori    In the region of the Orion nebula T-association.
V0378 Ori    In the region of the Orion nebula T-association.
V0379 Ori    In the region of the Orion nebula T-association.
V0380 Ori    In the nebula NGC 1999. In the region of the Orion
             nebula T-association. Spectrum description
             [04002]. OH, CH emission.
V0381 Ori    In the region of the Orion nebula T-association.
V0382 Ori    P var. MAX = 2431146 + 227.8d*E (JD2429300 - 31200);
             Mean period is given in the Table (JD2428100 - 33700).
V0383 Ori    In the region of the Orion nebula T-association.
V0384 Ori    In the region of the Orion nebula T-association.
V0385 Ori    In the region of the Orion nebula T-association.
V0386 Ori    In the region of the Orion nebula T-association.
V0387 Ori    In the region of the Orion nebula T-association.
V0388 Ori    In the region of the Orion nebula T-association.
V0389 Ori    In the region of the Orion nebula T-association.
V0390 Ori    In the region of the Orion nebula T-association.
V0391 Ori    In the region of the Orion nebula T-association.
V0393 Ori    In the region of the Orion nebula T-association.
V0394 Ori    In the region of the Orion nebula T-association.
V0395 Ori    In the region of the Orion nebula T-association.
V0396 Ori    In the region of the Orion nebula T-association.
V0397 Ori    In the region of the Orion nebula T-association.
V0398 Ori    In the region of the Orion nebula T-association.
V0399 Ori    In the region of the Orion nebula T-association.
V0400 Ori    In the region of the Orion nebula T-association.
V0401 Ori    In the region of the Orion nebula T-association.
V0402 Ori    In the region of the Orion nebula T-association.
V0403 Ori    In the region of the Orion nebula T-association.
V0404 Ori    In the region of the Orion nebula T-association.
V0405 Ori    In the region of the Orion nebula T-association.
V0406 Ori    In the region of the Orion nebula T-association.
V0407 Ori    In the region of the Orion nebula T-association.
V0408 Ori    In the region of the Orion nebula T-association.
V0409 Ori    In the region of the Orion nebula T-association.
V0410 Ori    In the region of the Orion nebula T-association.
V0411 Ori    In the region of the Orion nebula T-association.
V0412 Ori    In the region of the Orion nebula T-association.
V0413 Ori    In the region of the Orion nebula T-association.
V0414 Ori    In the region of the Orion nebula T-association.
V0415 Ori    In the region of the Orion nebula T-association.
V0416 Ori    In the region of the Orion nebula T-association.
V0417 Ori    In the region of the Orion nebula T-association.
V0418 Ori    In the region of the Orion nebula T-association.
V0419 Ori    In the region of the Orion nebula T-association.
V0420 Ori    In the region of the Orion nebula T-association.
V0421 Ori    In the region of the Orion nebula T-association.
V0422 Ori    In the region of the Orion nebula T-association.
V0423 Ori    In the region of the Orion nebula T-association.
V0424 Ori    In the region of the Orion nebula T-association.
V0425 Ori    In the region of the Orion nebula T-association.
V0426 Ori    In the region of the Orion nebula T-association.
V0427 Ori    In the region of the Orion nebula T-association.
V0428 Ori    In the region of the Orion nebula T-association.
V0432 Ori    Delta(S) = 0.
V0435 Ori    P var. Max = 2430350 + 186d*E (JD2429600 - 30730);
             Max = 2431373 + 186d*E (JD2431370 - 3250) [02279];
             since JD2434000 - see Table.
V0436 Ori    In the T-association CO Ori.
V0437 Ori    In the T-association CO Ori.
V0438 Ori    In the T-association CO Ori.
V0439 Ori    In the T-association CO Ori.
V0441 Ori    In the T-association CO Ori.
V0442 Ori    VB A (B 16.6m, 20", 73deg). In the T-association CO Ori.
V0443 Ori    In the T-association CO Ori.
V0444 Ori    In the T-association CO Ori.
V0445 Ori    In the T-association CO Ori.
V0446 Ori    In the T-association CO Ori.
V0447 Ori    In the T-association CO Ori.
V0448 Ori    In the T-association CO Ori.
V0449 Ori    In the T-association CO Ori.
             In [08289] was considered as an EW type variable with the
             elements: Min I = 2430259.622 + 0.441990d*E
             (JD2430250 - 5550), 14.8m - 15.7m pg.
V0450 Ori    In the T-association CO Ori.
V0452 Ori    In the T-association CO Ori.
V0453 Ori    In the T-association CO Ori.
V0454 Ori    In the T-association CO Ori.
V0455 Ori    In the T-association CO Ori.
V0456 Ori    In the T-association CO Ori.
V0457 Ori    In the T-association CO Ori.
V0458 Ori    In the T-association CO Ori.
V0460 Ori    In the T-association CO Ori.
V0461 Ori    In the T-association CO Ori.
V0463 Ori    In the T-association CO Ori.
V0464 Ori    In the T-association CO Ori.
V0465 Ori    In the T-association CO Ori.
V0466 Ori    In the region of the Orion nebula T-association.
V0467 Ori    In the T-association CO Ori.
V0468 Ori    In the region of the Orion nebula T-association.
V0470 Ori    In the region of the Orion nebula T-association. Star
             Pi 1411. Near to WY Ori = Pi 1396.
V0473 Ori    In the region of the Orion nebula T-association.
V0474 Ori    In the region of the Orion nebula T-association.
V0475 Ori    In the region of the Orion nebula T-association.
V0476 Ori    In the region of the open cluster lambda Ori.
V0477 Ori    In the region of the open cluster lambda Ori.
V0478 Ori    In the region of the Orion nebula T-association.
V0479 Ori    In the region of the Orion nebula T-association. In the
             infrared A>1.5m.
V0480 Ori    In the region of the Orion nebula T-association. In the
             infrared A>1.5m.
V0481 Ori    In the region of the Orion nebula T-association.
V0482 Ori    In the region of the Orion nebula T-association.
V0484 Ori    In the region of the Orion nebula T-association.
             In the infrared A>1.0m.
V0485 Ori    In the region of the Orion nebula T-association.
             In the infrared  A>1.0m.
V0486 Ori    In the region of the Orion nebula T-association.
V0487 Ori    In the region of the Orion nebula T-association.
V0489 Ori    In the region of the Orion nebula T-association.
             In the infrared A>1.0m.
V0490 Ori    In the region of the Orion nebula T-association.
             In the infrared A>1.0m.
V0491 Ori    In the region of the Orion nebula T-association.
             In the infrared A>1.0m.
V0492 Ori    In the region of the Orion nebula T-association.
             Northern component of the close pair of infrared stars.
             In the infrared A = 1m.
V0493 Ori    In the region of the Orion nebula T-association.
             In the infrared A>1.0m.
V0494 Ori    In the region of the Orion nebula T-association.
V0495 Ori    In the region of the Orion nebula T-association.
             Close binary (ro = 0.24"). It is unknown which of the
             components varies.
V0496 Ori    In the region of the Orion nebula T-association.
             In the infrared A>1.0m.
V0497 Ori    In the region of the Orion nebula T-association.
             In the infrared A>1.0m.
V0498 Ori    In the region of the Orion nebula T-association.
V0500 Ori    In the region of the Orion nebula T-association.
V0501 Ori    In the region of the Orion nebula T-association.
V0502 Ori    In the region of the Orion nebula T-association.
V0504 Ori    Min II 15.4.
V0505 Ori    In the region of the nebula IC 434.
V0507 Ori    In the region of the nebula IC 434.
V0508 Ori    In the region of the nebula IC 434.
V0509 Ori    In the region of the nebula IC 434.
V0510 Ori    In the region of the nebula IC 434.
V0511 Ori    In the region of the nebula IC 434.
V0514 Ori    In the region of the nebula IC 434.
V0516 Ori    Max = 2430325 + 139d*E (JD2430250 - 5350); P = 70d
             (JD2435350 - 550).
V0519 Ori    Min II 12.9.
V0522 Ori    In the region of the nebula IC 434.
V0523 Ori    In the region of the nebula IC 434.
V0525 Ori    Min II 14.7.
V0526 Ori    In the region of T-association FU Ori.
V0529 Ori    Nova Ori 1678?
             Recurrent outburst was possibly observed at 1894 [02866].
             Earlier the object was considered as nova Ori [1667
             2862, 2863, 2867, 2868], its existence being considered
             as doubtful [03813].
V0537 Ori    In the region of the open cluster lambda Ori.
V0538 Ori    In the region of the Orion nebula T-association.
V0539 Ori    In the region of the Orion nebula T-association.
V0540 Ori    In the region of the Orion nebula T-association.
V0541 Ori    In the region of the Orion nebula T-association.
V0542 Ori    In the region of the Orion nebula T-association.
V0544 Ori    In the region of the Orion nebula T-association.
V0545 Ori    In the region of the Orion nebula T-association.
V0546 Ori    In the region of the Orion nebula T-association.
V0547 Ori    In the region of the Orion nebula T-association.
V0548 Ori    In the region of the open cluster lambda Ori.
V0549 Ori    In the region of the open cluster lambda Ori.
V0550 Ori    In the region of the Orion nebula T-association.
V0551 Ori    In the region of the Orion nebula T-association.
V0552 Ori    In the region of the Orion nebula T-association.
V0553 Ori    In the region of the Orion nebula T-association.
V0554 Ori    In the region of the Orion nebula T-association.
V0555 Ori    In the region of the Orion nebula T-association.
V0556 Ori    In the region of the Orion nebula T-association.
V0557 Ori    In the region of the Orion nebula T-association.
V0559 Ori    In the region of the Orion nebula T-association.
V0560 Ori    In the region of the Orion nebula T-association.
V0561 Ori    In the region of the Orion nebula T-association.
V0562 Ori    In the region of the Orion nebula T-association.
V0563 Ori    In the region of the Orion nebula T-association.
V0564 Ori    In the region of the Orion nebula T-association.
V0565 Ori    In the region of the Orion nebula T-association.
V0566 Ori    In the region of the Orion nebula T-association.
V0567 Ori    In the region of the Orion nebula T-association.
V0568 Ori    In the region of the Orion nebula T-association.
V0569 Ori    In the region of the Orion nebula T-association.
V0570 Ori    In the region of the Orion nebula T-association.
V0571 Ori    In the region of the Orion nebula T-association.
V0572 Ori    In the region of the open cluster lambda Ori.
V0573 Ori    In the region of the Orion nebula T-association.
V0574 Ori    In the region of the Orion nebula T-association.
V0575 Ori    In the region of the Orion nebula T-association.
V0576 Ori    In the region of the Orion nebula T-association.
V0577 Ori    In the region of the Orion nebula T-association.
V0578 Ori    In the region of the Orion nebula T-association.
V0579 Ori    In the region of the Orion nebula T-association.
V0580 Ori    In the region of the Orion nebula T-association.
V0581 Ori    In the region of the Orion nebula T-association.
V0582 Ori    In the region of the Orion nebula T-association.
V0584 Ori    In the region of the Orion nebula T-association.
V0585 Ori    In the region of the Orion nebula T-association.
V0586 Ori    In the region of the Orion nebula T-association.
V0587 Ori    In the region of the Orion nebula T-association.
V0588 Ori    In the region of the Orion nebula T-association.
V0589 Ori    In the region of the Orion nebula T-association.
V0590 Ori    In the region of the Orion nebula T-association.
V0591 Ori    In the region of the Orion nebula T-association.
V0592 Ori    In the region of the Orion nebula T-association.
V0593 Ori    In the region of the Orion nebula T-association.
V0594 Ori    In the region of the Orion nebula T-association.
V0595 Ori    In the region of the nebula IC 434.
V0596 Ori    In the region of the open cluster lambda Ori.
V0597 Ori    In the region of the nebula IC 434.
V0598 Ori    In the region of the open cluster lambda Ori.
V0599 Ori    In the region of the Orion nebula T-association.
V0600 Ori    In the region of the nebula IC 434.
V0601 Ori    In the region of the nebula IC 434.
V0602 Ori    In the region of the nebula IC 434.
V0603 Ori    In the region of the nebula IC 434.
V0604 Ori    In the region of the nebula IC 434.
V0605 Ori    In the region of the nebula IC 434.
V0606 Ori    In the region of the nebula IC 434.
V0607 Ori    In the region of the nebula IC 434.
V0608 Ori    In the region of the nebula IC 434.
V0610 Ori    In the region of the nebula IC 434.
V0611 Ori    In the region of the nebula IC 434.
V0612 Ori    VB, SE-comp.; NW-comp.=NSV 02555. In the region of the
             nebula IC 434.
V0614 Ori    In the region of T-association FU Ori.
V0615 Ori    In the region of the nebula IC 434.
V0616 Ori    In the region of the nebula IC 434.
V0617 Ori    In the region of the nebula IC 434.
V0618 Ori    In the region of the nebula IC 434.
V0619 Ori    In the region of the nebula IC 434.
V0620 Ori    In the region of the nebula IC 434.
V0621 Ori    In the region of the nebula IC 434.
V0622 Ori    In the region of the nebula IC 434.
V0623 Ori    In the region of the nebula IC 434.
V0625 Ori    In the region of T-association FU Ori.
V0626 Ori    In the region of T-association FU Ori.
V0627 Ori    In the region of T-association FU Ori.
V0628 Ori    In the region of T-association FU Ori.
V0629 Ori    In the region of T-association FU Ori.
V0630 Ori    In the region of T-association FU Ori.
V0631 Ori    In the region of T-association FU Ori.
V0632 Ori    In the region of T-association FU Ori.
V0634 Ori    In the region of T-association FU Ori.
V0635 Ori    In the region of T-association FU Ori.
V0636 Ori    In the region of T-association FU Ori.
V0637 Ori    In the region of T-association FU Ori.
V0638 Ori    In the region of T-association FU Ori.
V0639 Ori    In the region of T-association FU Ori.
V0640 Ori    d <= 0.02P.
V0641 Ori    Min II 14.5.
V0642 Ori    d = 0.05P?.
V0643 Ori    P = 26.2075d?
V0647 Ori    Min II 11.9. P var. Min I = 2418005.035 + 0.977575d*E
             (JD2414660 - 23230); since JD2423230 - see Table.
V0648 Ori    Min II 12.2.
V0649 Ori    In the T-association CO - Ori. VB A (B 15m, 2", 0deg).
V0650 Ori    In the region of the open cluster lambda Ori.
V0652 Ori    In the region of the Orion nebula T-association.
V0654 Ori    In the region of the Orion nebula T-association.
V0655 Ori    In the region of the Orion nebula T-association.
V0656 Ori    In the region of the Orion nebula T-association.
V0657 Ori    In the region of the Orion nebula T-association.
V0658 Ori    In the region of the Orion nebula T-association.
V0659 Ori    In the region of the Orion nebula T-association.
V0667 Ori    Min II 15.0.
V0676 Ori    In the region of the Orion nebula T-association.
V0677 Ori    In the region of the Orion nebula T-association.
V0678 Ori    In the region of the Orion nebula T-association.
V0679 Ori    In the region of the Orion nebula T-association.
V0680 Ori    In the region of the Orion nebula T-association.
V0681 Ori    In the region of the Orion nebula T-association.
V0682 Ori    In the region of the Orion nebula T-association.
V0683 Ori    In the region of the Orion nebula T-association.
V0684 Ori    In the region of the Orion nebula T-association.
V0685 Ori    In the region of the Orion nebula T-association.
             A(U) = 1.0m.
V0686 Ori    In the region of the Orion nebula T-association.
V0687 Ori    In the region of the Orion nebula T-association.
V0688 Ori    In the region of the Orion nebula T-association.
V0689 Ori    In the region of the Orion nebula T-association.
V0690 Ori    In the region of the Orion nebula T-association.
V0691 Ori    In the region of the Orion nebula T-association.
V0692 Ori    In the region of the Orion nebula T-association.
V0693 Ori    In the region of the Orion nebula T-association.
V0694 Ori    In the region of the Orion nebula T-association.
V0695 Ori    In the region of the Orion nebula T-association.
V0696 Ori    In the region of the Orion nebula T-association.
V0697 Ori    In the region of the Orion nebula T-association.
V0698 Ori    In the region of the Orion nebula T-association.
V0699 Ori    In the region of the Orion nebula T-association.
V0700 Ori    In the region of the Orion nebula T-association.
V0701 Ori    In the region of the Orion nebula T-association.
V0702 Ori    In the region of the Orion nebula T-association.
V0703 Ori    In the region of the Orion nebula T-association.
V0704 Ori    In the region of the Orion nebula T-association.
V0705 Ori    In the region of the Orion nebula T-association.
V0706 Ori    In the region of the Orion nebula T-association.
V0707 Ori    In the region of the Orion nebula T-association.
V0708 Ori    In the region of the Orion nebula T-association.
V0709 Ori    In the region of the Orion nebula T-association.
V0710 Ori    In the region of the Orion nebula T-association.
V0711 Ori    In the region of the Orion nebula T-association.
V0712 Ori    In the region of the Orion nebula T-association.
V0713 Ori    In the region of the Orion nebula T-association.
             A(U) = 4.0m.
V0714 Ori    In the region of the Orion nebula T-association.
V0715 Ori    In the region of the Orion nebula T-association.
V0716 Ori    In the region of the Orion nebula T-association.
V0717 Ori    In the region of the Orion nebula T-association.
V0718 Ori    In the region of the Orion nebula T-association.
             Probably the sf-component of a very close pair.
V0719 Ori    In the region of the Orion nebula T-association.
V0720 Ori    In the region of the Orion nebula T-association.
V0721 Ori    In the region of the Orion nebula T-association.
V0722 Ori    In the region of the Orion nebula T-association.
V0723 Ori    In the region of the Orion nebula T-association.
V0724 Ori    In the region of the Orion nebula T-association.
V0725 Ori    In the region of the Orion nebula T-association.
V0726 Ori    In the region of the Orion nebula T-association.
V0727 Ori    In the region of the Orion nebula T-association.
V0728 Ori    In the region of the Orion nebula T-association.
V0729 Ori    In the region of the Orion nebula T-association.
V0730 Ori    In the region of the Orion nebula T-association.
V0731 Ori    In the region of the Orion nebula T-association.
V0732 Ori    In the region of the Orion nebula T-association.
V0733 Ori    In the region of the Orion nebula T-association.
V0734 Ori    In the region of the Orion nebula T-association.
V0735 Ori    In the region of the Orion nebula T-association.
V0736 Ori    In the region of the Orion nebula T-association.
V0737 Ori    In the region of the Orion nebula T-association.
             A(U) > 2.4m.
V0738 Ori    In the region of the Orion nebula T-association.
V0739 Ori    In the region of the Orion nebula T-association.
V0740 Ori    In the region of the Orion nebula T-association.
             A(pg) > 4.0m.
V0741 Ori    In the region of the Orion nebula T-association.
V0742 Ori    In the region of the Orion nebula T-association.
V0744 Ori    In the region of the Orion nebula T-association.
V0745 Ori    In the region of the Orion nebula T-association.
V0746 Ori    In the region of the Orion nebula T-association.
V0747 Ori    In the region of the Orion nebula T-association.
V0748 Ori    In the region of the Orion nebula T-association.
V0749 Ori    In the region of the Orion nebula T-association.
V0750 Ori    In the region of the Orion nebula T-association.
V0751 Ori    In the region of the Orion nebula T-association.
V0752 Ori    In the region of the Orion nebula T-association.
V0753 Ori    In the region of the Orion nebula T-association.
V0754 Ori    In the region of the Orion nebula T-association.
V0755 Ori    In the region of the Orion nebula T-association.
V0756 Ori    In the region of the Orion nebula T-association.
V0757 Ori    In the region of the Orion nebula T-association.
V0758 Ori    In the region of the Orion nebula T-association.
V0759 Ori    In the region of the Orion nebula T-association.
V0760 Ori    In the region of the Orion nebula T-association.
V0761 Ori    In the region of the Orion nebula T-association.
V0762 Ori    In the region of the Orion nebula T-association.
V0763 Ori    In the region of the Orion nebula T-association.
V0764 Ori    In the region of the Orion nebula T-association.
V0765 Ori    In the region of the Orion nebula T-association.
V0766 Ori    In the region of the Orion nebula T-association.
V0767 Ori    In the region of the Orion nebula T-association.
             A(U) = 1.5m.
V0768 Ori    In the region of the Orion nebula T-association.
V0770 Ori    In the region of the Orion nebula T-association.
V0771 Ori    In the region of the Orion nebula T-association.
V0772 Ori    In the region of the Orion nebula T-association.
V0773 Ori    In the region of the Orion nebula T-association.
V0774 Ori    In the region of the Orion nebula T-association.
V0775 Ori    In the region of the Orion nebula T-association.
V0776 Ori    In the region of the Orion nebula T-association.
V0777 Ori    In the region of the Orion nebula T-association.
V0778 Ori    In the region of the Orion nebula T-association.
             A(pg) = 1.6m.
V0779 Ori    In the region of the Orion nebula T-association.
V0780 Ori    In the region of the Orion nebula T-association.
             A(U) = 1.0m.
V0781 Ori    In the region of the Orion nebula T-association.
V0782 Ori    In the region of the Orion nebula T-association.
V0783 Ori    In the region of the Orion nebula T-association.
             A(pg) = 3.0m.
V0784 Ori    In the region of the Orion nebula T-association.
V0785 Ori    In the region of the Orion nebula T-association.
V0786 Ori    In the region of the Orion nebula T-association.
V0787 Ori    In the region of the Orion nebula T-association.
V0788 Ori    In the region of the Orion nebula T-association.
V0789 Ori    In the region of the Orion nebula T-association.
V0790 Ori    In the region of the Orion nebula T-association.
V0791 Ori    In the region of the Orion nebula T-association.
V0792 Ori    In the region of the Orion nebula T-association.
V0793 Ori    In the region of the Orion nebula T-association.
V0794 Ori    In the region of the Orion nebula T-association.
V0795 Ori    In the region of the Orion nebula T-association.
V0796 Ori    In the region of the Orion nebula T-association.
V0797 Ori    In the region of the Orion nebula T-association.
V0798 Ori    In the region of the Orion nebula T-association.
V0799 Ori    In the region of the Orion nebula T-association.
V0800 Ori    In the region of the Orion nebula T-association.
V0801 Ori    In the region of the Orion nebula T-association.
V0802 Ori    In the region of the Orion nebula T-association.
V0803 Ori    In the region of the Orion nebula T-association.
V0804 Ori    In the region of the Orion nebula T-association.
V0805 Ori    In the region of the Orion nebula T-association.
V0806 Ori    In the region of the Orion nebula T-association.
V0807 Ori    In the region of the Orion nebula T-association.
V0808 Ori    In the region of the Orion nebula T-association.
V0810 Ori    In the region of the Orion nebula T-association.
V0811 Ori    In the region of the Orion nebula T-association.
V0812 Ori    In the region of the Orion nebula T-association.
V0813 Ori    In the region of the Orion nebula T-association.
V0814 Ori    In the region of the Orion nebula T-association.
V0815 Ori    In the region of the Orion nebula T-association.
V0816 Ori    In the region of the Orion nebula T-association.
V0817 Ori    In the region of the Orion nebula T-association.
V0818 Ori    In the region of the Orion nebula T-association.
V0819 Ori    In the region of the Orion nebula T-association.
V0820 Ori    In the region of the Orion nebula T-association.
V0821 Ori    In the region of the Orion nebula T-association.
V0822 Ori    In the region of the Orion nebula T-association.
V0823 Ori    In the region of the Orion nebula T-association.
V0824 Ori    In the region of the Orion nebula T-association.
V0825 Ori    In the region of the Orion nebula T-association.
V0826 Ori    In the region of the Orion nebula T-association.
V0827 Ori    In the region of the Orion nebula T-association.
V0828 Ori    In the region of the Orion nebula T-association.
V0829 Ori    In the region of the Orion nebula T-association.
V0830 Ori    In the region of the Orion nebula T-association.
V0831 Ori    In the region of the Orion nebula T-association.
V0832 Ori    In the region of the Orion nebula T-association.
V0833 Ori    In the region of the Orion nebula T-association.
V0834 Ori    In the region of the Orion nebula T-association.
V0835 Ori    In the region of the Orion nebula T-association.
V0836 Ori    In the region of the Orion nebula T-association.
             A(U) > 1.5m.
V0837 Ori    In the region of the Orion nebula T-association.
V0838 Ori    In the region of tbe Orion nebula T-association.
V0839 Ori    In the region of tbe Orion nebula T-association.
V0840 Ori    In the region of the Orion nebula T-association.
             A(pg) = 0.7m.
V0841 Ori    In the region of the Orion nebula T-association.
V0842 Ori    In the region of the Orion nebula T-association.
V0843 Ori    In the region of the Orion nebula T-association.
V0844 Ori    In the region of the Orion nebula T-association.
V0845 Ori    In the region of the Orion nebula T-association.
V0846 Ori    In the region of the Orion nebula T-association.
V0847 Ori    In the region of the Orion nebula T-association.
V0848 Ori    In the region of the Orion nebula T-association.
V0849 Ori    In the region of the Orion nebula T-association.
V0850 Ori    In the region of the Orion nebula T-association.
V0851 Ori    In the region of the Orion nebula T-association.
V0852 Ori    In the region of the Orion nebula T-association.
V0853 Ori    In the region of the Orion nebula T-association.
V0854 Ori    In the region of the Orion nebula T-association.
V0855 Ori    In the region of the Orion nebula T-association.
             A(U) > 2.0m.
V0856 Ori    In the region of the Orion nebula T-association.
V0857 Ori    In the region of the Orion nebula T-association.
             A(pg) > 5.0m.
V0858 Ori    In the region of the Orion nebula T-association.
V0859 Ori    In the region of the Orion nebula T-association.
V0860 Ori    In the region of the Orion nebula T-association.
V0861 Ori    In the region of the Orion nebula T-association.
V0862 Ori    In the region of the Orion nebula T-association.
V0863 Ori    In the region of the Orion nebula T-association.
V0864 Ori    In the region of the Orion nebula T-association.
V0865 Ori    In the region of the Orion nebula T-association.
V0866 Ori    In the region of the Orion nebula T-association.
V0867 Ori    In the region of the Orion nebula T-association.
             A(pg)>3.0m.
V0868 Ori    In the region of the Orion nebula T-association.
V0869 Ori    In the region of the Orion nebula T-association.
V0870 Ori    In the region of the Orion nebula T-association.
V0871 Ori    In the region of the Orion nebula T-association.
V0872 Ori    In the region of the Orion nebula T-association.
V0873 Ori    In the region of the Orion nebula T-association.
V0874 Ori    In the region of the Orion nebula T-association.
V0875 Ori    In the region of the Orion nebula T-association.
V0876 Ori    In the region of the Orion nebula T-association.
             Southem component of a close pair.
V0877 Ori    In the region of the Orion nebula T-association.
V0878 Ori    In the region of the Orion nebula T-association.
V0879 Ori    In the region of the Orion nebula T-association.
V0880 Ori    In the region of the Orion nebula T-association.
V0881 Ori    In the region of the Orion nebula T-association.
V0882 Ori    In the region of the Orion nebula T-association.
V0883 Ori    In the region of the Orion nebula T-association.
             In the apex of a cometary nebula.
V0884 Ori    In the region of the Orion nebula T-association.
V0885 Ori    In the region of the Orion nebula T-association.
V0886 Ori    In the region of the Orion nebula T-association.
             A(pg) > 3.5m.
V0888 Ori    In the region of the Orion nebula T-association.
V0889 Ori    In the region of the Orion nebula T-association.
V0890 Ori    In the region of the Orion nebula T-association.
V0891 Ori    In the region of the Orion nebula T-association.
V0892 Ori    In the region of the Orion nebula T-association.
             Southern component of a pair (ro = 3").
V0893 Ori    In the region of the Orion nebula T-association.
             A(U) = 2.0m.
V0894 Ori    In the region of the Orion nebula T-association.
V0895 Ori    In the region of the Orion nebula T-association.
V0896 Ori    In the region of the Orion nebula T-association.
V0897 Ori    In the region of the Orion nebula T-association.
V0898 Ori    In the region of the Orion nebula T-association.
V0899 Ori    In the region of the Orion nebula T-association.
V0900 Ori    In the region of the Orion nebula T-association.
             A(pg) > 2.5m.
V0901 Ori    In the region of the nebula IC 434.
V0902 Ori    In the region of the Orion nebula T-association.
V0904 Ori    In the region of the Orion nebula T-association.
V0905 Ori    In the region of the Orion nebula T-association.
V0906 Ori    In the region of the Orion nebula T-association.
V0907 Ori    In the region of the Orion nebula T-association.
V0908 Ori    In the region of the Orion nebula T-association.
V0909 Ori    In the region of the Orion nebula T-association.
V0916 Ori    P = 0.28297d? Member of the open cluster NGC 2169.
V0917 Ori    Member of the open cluster NGC 2169.
V0918 Ori    In the region of the Orion nebula T-association.
V0919 Ori    In the region of the Orion nebula T-association.
V0920 Ori    In the region of the Orion nebula T-association.
V0921 Ori    In the region of the Orion nebula T-association.
V0922 Ori    In the region of the Orion nebula T-association.
V0923 Ori    In the region of the Orion nebula T-association.
V0924 Ori    In the region of the Orion nebula T-association.
V0926 Ori    In the region of the Orion nebula T-association.
V0927 Ori    In the region of the Orion nebula T-association.
V0928 Ori    In the region of the Orion nebula T-association.
V0929 Ori    In the region of the Orion nebula T-association.
V0930 Ori    In the region of the Orion nebula T-association.
V0931 Ori    In the region of the Orion nebula T-association.
V0932 Ori    In the region of the Orion nebula T-association.
V0933 Ori    In the region of the Orion nebula T-association.
V0934 Ori    In the region of the Orion nebula T-association.
V0935 Ori    In the region of the Orion nebula T-association.
V0937 Ori    In the region of the Orion nebula T-association.
V0938 Ori    In the region of the Orion nebula T-association.
V0939 Ori    In the region of the Orion nebula T-association.
V0941 Ori    In the region of the Orion nebula T-association.
V0942 Ori    In the region of the Orion nebula T-association.
V0943 Ori    In the region of the Orion nebula T-association.
V0945 Ori    In the region of the Orion nebula T-association.
V0946 Ori    In the region of the Orion nebula T-association.
V0947 Ori    In the region of the Orion nebula T-association.
V0948 Ori    In the region of the Orion nebula T-association.
V0949 Ori    In the region of the Orion nebula T-association.
V0950 Ori    In the region of the Orion nebula T-association.
V0951 Ori    In the region of the Orion nebula T-association.
V0952 Ori    In the region of the Orion nebula T-association.
V0953 Ori    In the region of the nebula IC 434.
V0956 Ori    In the region of the nebula IC 434.
V0957 Ori    In the region of the nebula IC 434.
V0958 Ori    In the region of the Orion nebula T-association.
V0960 Ori    In the region of the nebula IC 434.
V0961 Ori    In the region of the Orion nebula T-association.
V0964 Ori    P var. Max = 2415800.389 + 0.5046772d*E
             (JD2415800 - 21010); Max = 2424500.446 + 0.50466477d*E
             (JD2424500 - 30500); since JD2431500 - see Table.
V0966 Ori    In the region of the Orion nebula T-association.
V0967 Ori    In the region of the Orion nebula T-association.
V0968 Ori    In the region of the Orion nebula T-association.
V0969 Ori    In the region of the Orion nebula T-association.
V0970 Ori    In the region of the Orion nebula T-association.
V0971 Ori    In the region of the Orion nebula T-association.
V0972 Ori    In the region of the Orion nebula T-association.
V0973 Ori    In the region of the Orion nebula T-association.
V0974 Ori    In the region of the Orion nebula T-association.
V0975 Ori    In the region of the Orion nebula T-association.
V0976 Ori    In the region of the Orion nebula T-association.
V0977 Ori    In the region of the Orion nebula T-association.
V0978 Ori    In the region of the Orion nebula T-association.
V0979 Ori    In the region of the Orion nebula T-association.
V0980 Ori    In the region of the Orion nebula T-association.
V0981 Ori    In the region of the Orion nebula T-association.
V0982 Ori    In the region of the Orion nebula T-association.
V0983 Ori    In the region of the Orion nebula T-association.
V0984 Ori    In the region of the Orion nebula T-association.
V0985 Ori    In the region of the Orion nebula T-association.
V0986 Ori    In the region of the Orion nebula T-association.
V0987 Ori    In the region of the Orion nebula T-association.
V0988 Ori    In the region of the Orion nebula T-association.
V0989 Ori    In the region of the Orion nebula T-association.
V0990 Ori    In the region of the Orion nebula T-association.
V0991 Ori    In the region of the Orion nebula T-association.
V0992 Ori    In the region of the Orion nebula T-association.
V0994 Ori    In the region of the Orion nebula T-association.
V0995 Ori    In the region of the Orion nebula T-association.
V0996 Ori    In the region of the Orion nebula T-association.
V0997 Ori    In the region of the Orion nebula T-association.
V0998 Ori    mu = 0.28", ro = 221deg.
V0999 Ori    In the region of the Orion nebula T-association.
V1000 Ori    In the region of the Orion nebula T-association.
V1001 Ori    In the region of the Orion nebula T-association.
V1002 Ori    In the region of the Orion nebula T-association.
V1003 Ori    mu = 0.272", ro = 60.8deg.
V1004 Ori    VB A (B 10.57m, 37", 204deg); SB (P = 2.74d).
V1005 Ori    The range of light variations (characteristic for BY Dra
             type variability) between the flares is given in the Table;
             the amplitude of the flares A(U) can reach 3.2m.
V1006 Ori    In the region of the Orion nebula T-association.
V1007 Ori    In the region of the Orion nebula T-association.
V1016 Ori    In the region of the Orion nebula T-association.
             In the cluster NGC 1976. Orion Trapezium
             member: teta1 Ori A (B = BM Ori, 8.7", 32deg; C 5.13m,
             13.1", 131deg; D 6.70m, 21.6", 96deg). d = 0.001P.
V1017 Ori    In the region of the Orion nebula T-association.
V1018 Ori    In the region of the Orion nebula T-association.
V1019 Ori    In the region of the Orion nebula T-association.
V1020 Ori    In the region of the Orion nebula T-association.
V1022 Ori    In the region of T-association FU Ori.
V1028 Ori    P = 6d?
V1029 Ori    In the region of the Orion nebula T-association.
V1030 Ori    In the region of the nebula IC 434. (sig Ori) E
             (A 4.1m; B 5.1m, A = 0.247", P = 170yr; C 8.79m, 11.2",
             238deg; D 6.66m, 12.9", 84deg; E 41.6", 61deg). Min I
             (HeI) = 2442802.48 + 1.19080d*E. Unusual helium variable.
             Epoch of Min I brightness is given in the Table
             (Min II 6.71, Min II - Min I = 0.43P). This epoch is being
             observed by 0.18P later than the epoch of minimum strength
             of the HeI lambda 4026 A line. According to [09524], light
             minima are due to "eclipses" of the star surface
             by two isolated clouds (consisting of hydrogen and
             helium), which are located almost oppositely near
             the intersections of the magnetic And rotational
             equator.
V1031 Ori    VB (0.159", 104deg, 1980.7). Min II 6.32; DII = 0.017P.
V1034 Ori    Epoch of light minimum is given.
V1035 Ori    In the region of the Orion nebula T-association.
V1036 Ori    In the region of the Orion nebula T-association.
V1037 Ori    In the region of the Orion nebula T-association.
V1038 Ori    In the region of the Orion nebula T-association.
V1039 Ori    In the region of the Orion nebula T-association.
V1040 Ori    In the region of the Orion nebula T-association.
V1041 Ori    In the region of the Orion nebula T-association.
V1042 Ori    In the region of the Orion nebula T-association.
V1043 Ori    In the region of the Orion nebula T-association.
V1044 Ori    In the region of the Orion nebula T-association.
V1045 Ori    In the region of the Orion nebula T-association.
V1046 Ori    In the region of the Orion nebula T-association.
             SB 1. Min II 6.58. Possibly an ellipsoidal variable, its
             light variations being superimposed by light variations of
             the primary component of SX Ari type:
             Min (HeI) = 2442812.23 + 0.9015d*E [08054].
V1047 Ori    In the region of the Orion nebula T-association.
V1048 Ori    In the region of the Orion nebula T-association.
V1049 Ori    In the region of the Orion nebula T-association.
V1050 Ori    In the region of the Orion nebula T-association.
V1052 Ori    In the region of the Orion nebula T-association.
V1053 Ori    In the region of the Orion nebula T-association.
V1054 Ori    Epoch of light minimum is given. P = 8.596d?, P = 8.674d?
V1055 Ori    P(X) = 5.2d [09528].
V1056 Ori    VB A (B 9.8m, 28.7", 58deg).
V1058 Ori    In the region of the Orion nebula T-association.
V1059 Ori    In the region of the Orion nebula T-association.
V1060 Ori    In the region of the Orion nebula T-association.
V1061 Ori    In the region of the Orion nebula T-association.
V1062 Ori    In the region of the Orion nebula T-association.
V1063 Ori    In the region of the Orion nebula T-association.
V1064 Ori    In the region of the Orion nebula T-association.
V1065 Ori    In the region of the Orion nebula T-association.
V1066 Ori    In the region of the Orion nebula T-association.
V1067 Ori    In the region of the Orion nebula T-association.
V1068 Ori    In the region of the Orion nebula T-association.
V1069 Ori    In the region of the Orion nebula T-association.
V1070 Ori    In the region of the Orion nebula T-association.
V1071 Ori    In the region of the Orion nebula T-association.
V1072 Ori    In the region of the Orion nebula T-association.
V1073 Ori    In the region of the Orion nebula T-association.
V1074 Ori    In the region of the Orion nebula T-association.
V1075 Ori    In the region of the Orion nebula T-association.
V1076 Ori    In the region of the Orion nebula T-association.
V1077 Ori    In the region of the Orion nebula T-association.
V1078 Ori    In the region of the Orion nebula T-association.
V1079 Ori    In the region of the Orion nebula T-association.
V1080 Ori    In the region of the Orion nebula T-association.
V1081 Ori    In the region of the Orion nebula T-association.
V1082 Ori    In the region of the Orion nebula T-association.
V1083 Ori    In the region of the Orion nebula T-association.
V1084 Ori    In the region of the Orion nebula T-association.
V1377 Ori    SB?, Porb ~ 5.5 to 6.5d.
V1380 Ori    In a bright nebula.
alf   Ori    VB A (B 14.5m, 39.8", 110deg). Min = 2410600 + 2070d*E
             (1840 - 1929) [01012]. Since 1929 - see Table.
             The main variation is superimposed by the waves
             with P = 200 - 400d. Dust-gaseous shell (r = 50")
             [09529].
del   Ori    VB A (A 0.217", 144deg, 1980; B 14.0m, 33.1", 227deg;
             C 6.84m, 53.5", 359deg). Orion Belt cluster member.
             Min II 2.20.
             Apsidal motion (P = 210 yr). Shape of the light curve
             varies. The intrinsic brightness variability of the
             components is possible.
eps   Ori    Orion Belt cluster member.
eta   Ori    VB Aab (AC 0.037", 111deg, 1979.0, P = 9.219 yr [09535];
             B 4.8m, 1.60", 76deg, 1976.0; C 9.4m, 115", 51deg). EA/DM.
             Min II 3.57. The range of combined light variation of the
             components AAb (SB 2, P = 7.989268d), AC, and B is given
             in the Table. Outside eclipses there are sinusoidal light
             variations of the system with A(V) = 0.05m due to
             pulsations of the component Ab [09535] with P = 0.30197d
             [09536] or 0.30145d [09537]. According to [08566] these
             variations were not observed between 1970 and 1976.
pi  5 Ori    Min II 3.73. The period is improved using radial
             velocities [04627].
psi   Ori    VB A (B 11.1m, 2.7", 323deg; C 13.88m, 83", 196deg).
             Min II 4.58. The period is determined on the base of
             radial velocities [09541].
R     Pav    Pvar. Max = 2411219 + 228.34d (JD2411000 - 18500);
             Max = 2418527 + 230.95d*E (JD2418500 - 30000);
             since JD2430000 - see Table.
S     Pav    P var. Max = 2421479 + 389.64d*E(JD2421000 - 31000);
             since JD2431000 - see Table. Delta(m) var strongly.
             Min II is sometimes observed after Max I.
T     Pav    P var. Max = 2413328 + 243.45d*E(JD2405700 -
             25500); Max = 2425499 + 245.11d*E(JD2425500 -
             32500); since JD2432500 - see Table.
V     Pav    VBA (B 14.0m vis, 15", 327deg). Mean brightness var,
             P2 = 3735d, 9.7m - 10.7m.
W     Pav    P var. Before JD2431000 Max = 2413778 + 282.92d*E;
             since JD2431000 - see Table.
RT    Pav    Mean light var, 10.4m - 11.1m  1649, P2 = 757d.
SU    Pav    P var. Max = 2430036 + 245.18d*E (JD2411000 - 30100)
             [00001]; during JD247700 - 40000 - see Table.
SX    Pav    mu alpha = +0.0166s, mu delta = -0.05".
TW    Pav    Before JD2420400 Max = 2417760 + 397.d*E.
YY    Pav    Delta(m) var strongly. P possibly is twice longer, in that
             case Min II 14.4.
AR    Pav    Depth of eclipses Delta(m) = 2m B, d = 0.05P. Expanding
             shell.
BD    Pav    Only one outburst was observed [00629]. Brightness
             flickering. Eclipses according to the elements
             Min I = 2444412.676 + 0.1793015d*E, Delta(m) ~0.5m [09191].
             Outside outburst, 15.40m - 16.21m.
BF    Pav    Min II 11.9.
BI    Pav    Min II (Delta(m) ~0.05m) is possible.
DF    Pav    Epoch of min is given. Light curve shape strongly var.
DN    Pav    Delta(S) = 8:.
DW    Pav    Min II 16.3.
EG    Pav    Twice shorter P is possible [00001].
EL    Pav    Min II 15.5.
EN    Pav    Elements need confirmation.
EQ    Pav    Red.
FY    Pav    Min II? JD2436784.37.
HL    Pav    Blazhko effect?
HP    Pav    Min II 15.5.
HQ    Pav    Min II 12.7.
HY    Pav    Min II 12.1.
IL    Pav    RRC type is possible.
KR    Pav    Min II 14.1.
KZ    Pav    VB A (B 8.7m, 6.7", 119deg, 1971; C 9.2m, BC 1.0", 329deg,
             1971). P var. Min = 2430448.617 + 0.949880d*E
             (JD2416000 - 30000) [00001]; since JD2430000 - see Table.
             Min II is present.
LL    Pav    Min II 15.1.
LO    Pav    Min II 16.5.
LR    Pav    Min II 15.3.
LT    Pav    Min II 12.2.
LV    Pav    Min II 14.3.
LY    Pav    Min II 14.9.
MQ    Pav    Epoch of Min is given. EW/KW type with twice longer P is
             possible.
MR    Pav    Possible elements Max = 2436731.40 + 0.3737d*E [00001].
MS    Pav    Min II 14.1.
MW    Pav    d = 0.08P. Min II 8.92, dII = 0.11P.
NP    Pav    Deep Min II.
NW    Pav    [A/H] = -0.7.
OY    Pav    The chart in [06286] is wrong.
V0382 Pav    Type EW: is also possible.
kap   Pav    P var. Max = 2419619.38 + 9.0898d*E (JD2411930 - 22550);
             Max = 2425987.12 + 9.1028d*E (JD2422550 - 26980);
             Max = 2430530.67 + 9.0833d*E (JD2426980 - 31345);
             Max = 2433239.87 + 9.0956d*E (JD2431345 - 34045);
             Max = 2434693.11 + 9.0653d*E (JD2434045 - 37000);
             since JD2440000 - see Table. [Fe/H] = 0.0/ - 0.4.
             Moderately high Z coordinate (IZI ~240 pc provided
             the period - luminosity relation for DCEP stars is valid),
             low radial velocity. The period is not typical
             for CW stars. Ca II emission was noticed in the spectrum.
lam   Pav    VB A (B 12.4m, 63.1", 206deg).
rho   Pav    The main light variation P1 (see Table) with a
             semiamplitude delta(y) = 0.0069m is superposed by
             oscillations with P2 = 0.1131d (delta(y) = 0.0031m),
             P3 = 0.1612d (delta(y) = 0.0029m).
R     Peg    OH, H2O, SiO maser. P var. Max = 2396327 + 381.9d*E
             (JD2396300 - 2408200); Max = 2413012 + 371.4d*E
             (JD2413000 - 19800); Max = 2420092 + 379.77d*E
             (JD2420000 - 31100) [00960]; since JD2431100 - see Table.
T     Peg    P var. Max = 2398452 + 371.0d*E (JD2398400 - 2408900);
             Max = 2413697 + 386.8d*E (JD2413600 - 18700);
             Max = 2421016 + 362.5d*E (JD2420900 - 28000) [00960];
             Max = 2434343 + 376.0d*E (JD2428300 - 34300);
             Max = 2440984 + 368.7d*E (JD2434300 - 41000);
             since JD2441000 - see Table.
U     Peg    Min II 9.73. P var.
             There is a square term in the elements:
             -2.468D*10**(-11)*E**2.
             0 - C = 0.00323d*sin((2pi/16330)E + 0.418pi). Shape of
             the light curve varies.
W     Peg    SiO maser. P var. Max = 2413819 + 343.2d*E
             (JD2413800 - 26600); Max = 2427162 + 345.5d*E
             (JD2426600 - 32100) [00960]; Max = 2439690 + 348.75d*E
             (JD2432300 - 39700) [00001]; since JD2441400 - see Table.
X     Peg    P var. Max = 2414713 + 200.3d*E (JD2414700 - 21300);
             Max = 2420105 + 204.3d*E (JD2420100 - 23800);
             Max = 2423570 + 199.8d*E (JD2423600 - 31000) [00960];
             Max = 2432006 + 208d*E (JD2431000 - 32100);
             Max = 2434206 + 200.0d*E (JD2432100 - 39300);
             since JD2438400 - see Table.
Z     Peg    P var. Max = 2415433 + 318.9d*E (JD2398800 - 2420550);
             Max = 2420207 + 328.0d*E (JD2420200 - 32000) [00960];
             Max = 2432005 + 325.8d*E (JD2432000 - 37900);
             Max = 2437870 + 319d*E (JD2437500 - 40100);
             Max = 2442086 + 328.0d*E (JD2440100 - 43100);
             since JD2442100 - see Table.
RR    Peg    P var. Max = 2417582 + 268.3d*E (JD2416700 - 17850)
             [00001]; Max = 2417859 + 260.8d*E (JD2417850 - 21000)
             [00960]; since JD2421000 - see Table.
RS    Peg    P var. Max = 2415846 + 431.5d*E (JD2415800 - 18450);
             Max = 2418434 + 404.1d*E (JD2418400 - 24200);
             Max = 2424514 + 413.4d*E (JD2424500 - 34900) [00960];
             Max = 2436496 + 403.4d*E (JD2435700 - 38600) [00001];
             since JD2438500 - see Table.
RT    Peg    VB A (B 10.5m, 15.6", 291deg). P var.
             Max = 2423609 + 215.0d*E (JD2416000 - 24300);
             Max = 2428149 + 216.6d*E (JD2424300 - 32100);
             since JD2432100 - see Table.
RU    Peg    VB A (B 12.5m, 12", 18deg); SB2 (Porb = 0.3746d [09570]).
             There are also light oscillations with P = 11.6s
             and 50s [09571].
RV    Peg    Emission. Light curve (1907 - 1973) [09572]. P var.
             Max = 2428735 + 388.4d*E (JD2417000 - 32640);
             Max = 2430680 + 390.9d*E (JD2430200 - 38900);
             since JD2438800 - see Table.
RW    Peg    P var. Max = 2419393 + 208.4d*E (JD2412700 - 19400);
             Max = 2421520 + 213.0d*E (JD2419390 - 21550);
             Max = 2427133 + 208.0d*E (JD2421500 - 27150);
             since JD2427300 - see Table.
RX    Peg    P2 = 110d:.
RY    Peg    VB B (A = RZ Peg; B 20", 252deg).
RZ    Peg    VB A (B = RY Peg:20", 252deg). SC 6/9 - e. P var.
             Max = 2423361 + 441.4d*E (JD2411400 - 26450);
             Max = 2431215 + 434.0d*E (JD2426400 - 33000);
             since JD2433000 - see Table.
SS    Peg    P var. Max = 2416390 + 410.8d*E (JD2415500 - 20000);
             Max = 2422235 + 423.8d*E (JD2420000 - 27000);
             Max = 2427270 + 403.4d*E (JD2427000 - 29000);
             Max = 2437218 + 416.35d*E (JD2428500 - 43000);
             since JD2443000 - see Table.
SV    Peg    H2O emission.
SX    Peg    S 2.5/6 e. P var. Max = 2436043 + 306.56d*E
             (JD2414800 - 38300); since JD2438300 - see Table.
TU    Peg    P var. Max = 2417800 + 320.8d*E (JD2404300 - 18450);
             Max = 2420730 + 328.4d*E (JD2418450 - 20800);
             Max = 2428080 + 319.6d*E (JD2420800 - 31600);
             since JD2432800 - see Table.
TW    Peg    H2O maser. The basic light variation with the period given
             in the Table is superimposed by small oscillations
             with P = 94.13d.
TY    Peg    Min II 10.2. P var. Min I hel = 2419520.476 +
             3.0922754d*E (JD2412300 - 19600) [02389]; Min I hel =
             2425918.348 + 3.092252d*E (JD2419600 - 26000)
             [00001]; since JD2426000 - see Table.
TZ    Peg    P var? Max = 2425892 + 213.7d*E (JD2410000 - 28000);
             since JD2430000 - see Table.
UU    Peg    OH, H2O maser.
UW    Peg    According to [08837] P = 60d.
UX    Peg    P var. Min = 2428428.386 + 1.544618d*E (JD2422100 -
             28430) [00230]; Min = 2431273.597 + 1.544632d*E
             (JD2428420 - 34000) [00001]; since JD2434000 - see Table.
VV    Peg    Delta(S) = 8. P var. Max = 2420105.296 + 0.48837765d*E
             (JD2420000 - 28900); Max = 2433217.268 + 0.48838307d*E
             (JD2432800 - 38000) [03506]; since JD2438000 - see Table.
VW    Peg    P = 2.341295d?
VX    Peg    The basic light variation is superimposed by the secondary
             one with P = 80 - 90d:.
VZ    Peg    [Fe/H] = -1.75.
WW    Peg    P var. Max = 2433142 + 371.6d*E (JD2415670 - 33200)
             [00001]; since JD2436800 - see Table.
ZZ    Peg    Min II 12.5.
AE    Peg    P var. Max = 2415470.866 + 0.4967388d*E (JD2415500 -
             21000); Max = 2426161.544 + 0.496725d*E (JD2425400 -
             31500); Max = 2432632.809 + 0.496692d*E (JD2431500 -
             36000) [00001]; during JD2436000 - 40000 - see Table.
             Delta(S) = 6.3.
AG    Peg    SB2 (Porb = 820d [09580]).
             Maximum of brightness was in 1870, then the very
             slow light decrease was observed that was superimposed
             since 1935 by periodical light oscillations with
             A = 0.4m V
             and P = Porb: Min = 2428250 + 827.d*E ( JD2428000-43000)
             [09587]. After JD2442300 the period probably has changed:
             Min = 2442370 + 760d*E [09587]. In 1962 - 1979 the range of
             brightness was 7.95m - 8.55m V; M - m = 0.50P.
             Light minima correspond to the epochs of inferior
             conjunction of M 3 III component. Spectrum var: Beq
             (1893 - 1919); since 1922 the spectrum is symbiotic one,
             the M star spectrum being more noticeable.
             Surrounded by a radio nebula with 1" half-power diameter.
AN    Peg    P var. Max = 2428045 + 274.1d*E (JD2424500 - 38500)
             [09581]; since JD2438500 - see Table.
AO    Peg    Delta(S) = 4.3.
AQ    Peg    Min II 10.47; d = 0.030P. P var. Min I = 2424749.335 +
             5.548419d*E (JD2424000 - 34000) [00980];
             since JD2434000 - see Table.
AS    Peg    Of the two stars circled in the chart in [06286], the southern
             component varies.
AT    Peg    Min II 9.04. P var. Min I = 2425862.337 + 1.1460988d*E
             (JD2425800 - 37500) [00001]; Min I = 2437497.542 +
             1.146080d*E (JD2437490 - 40000) [06101]; Min I =
             2440407*4370 + 1.1461007d*E (JD2440000 - 42400)
             [00001]; since JD2442400 - see Table.
AU    Peg    Cepheid in a close binary system.
             SB1 (Porb = 53.319d, K1 = 41.8 km/s, gamma = -4.1 km/s,
             E = 0.12 [09582]). [Fe/H] = 0.1.
             P var. Max = 2428729.76 + 2.3978d*E (JD2426500 - 28750)
             [00916]; Max = 2433151.976 + 2.38934d*E (JD2433150 - 35800);
             Max = 2439039.08 + 2.39079d*E (JD2435800 - 39100) [00001];
             since JD2441700 - see Table.
             There is a square term in the elements given in the Table:
             +2.246d*10**(-6)*E**2. The shape of the light curve varies:
             0.20P <  M - m < 0.47P.
AV    Peg    P var. Max = 2416347.713 + 0.39036510d*E
             (JD2414000 - 26500) [00752]; Max = 2426582.301 +
             0.39037015d*E (JD2426500 - 36000) [09584];
             since JD2436000 - see Table. [Fe/H] = +0.02.
AW    Peg    d = 0.07P, Min II 7.60.
BB    Peg    Depth of Min II 0.60m.
             There is a square term in the elements given in the Table:
             +2.3d*10**(-11)*E**2. dI = 0.05P; dII = 0.00P.
BF    Peg    P var. Max = 2426589.293 + 0.495796d*E + 2.8d*10**(-9)*E**2
             (JD2426500 - 28800) [00522]; Max = 2433200.312 +
             0.495796d*E (JD2429400 - 33200) [00001]; Max =
             2437583.343 + 0.495674d*E (JD2437500 - 39400)
             [00001]; since JD2442650 - see Table.
BG    Peg    P var. Min = 2427386.3705 + 1.952452d*E (JD2426000 - 35000)
             [03567]; Min = 2436453.509 + 1.95238d*E (JD2435000 - 43500)
             [03624]; since JD2443500 - see Table.
BH    Peg    P var. Max = 2426596.535 + 0.64101381d*E
             (JD2426500 - 28200) [01038]; since JD2434400 - see Table.
             Blazhko effect. A var.
             Max (O - C) = 2442929.03 + 39.8d*N [09588]. (k - b)2 = 0.09;
             Delta(S) = 5.
BI    Peg    Waves with a cycle of 60 - 80d are superimposed.
BK    Peg    Min II 10.47.
BO    Peg    Min II 11.6. P var. Min I = 2427655.460 + 0.5804342d*E
             (JD2426500 - 35100) [02263]; since JD2444000 - see Table.
BP    Peg    P1 = 0.084510d; P1:P0 = 0.77. Beat
             period Pb = 0.3698d [06604].
BU    Peg    Observations are represented by the elements in the
             intervals JD2432000 - 34000, JD2438200 - 41400.
BX    Peg    Depth of Min II 0.62m; dI = 0.05P; dII = 0.00P.
             P var. Min I = 2431323.278 + 0.2804238d*E
             (JD2424700 - 39000) [00279]; since JD2439000 - see Table.
BY    Peg    P var. Min I = 2424745.75 + 0.34193403d*E
             (JD2424700 - 35400); since JD2435000 - see Table.
CC    Peg    Min II 12.9.
CG    Peg    Delta(S) = 2. P var?
CU    Peg    d = 0.010P. P var. Min = 2433895.463 + 3.8801345d*E
             (JD2425500 - 34000) [00001]; Min = 2434221.392 +
             3.880196d*E (JD2434000 - 36500) [07929];
             since JD2436500 - see Table.
CZ    Peg    Min II 13.9.
DF    Peg    Min II 9.2.
DG    Peg    P var. Max = 2425857 + 148.15d*E (JD2425500 -
             33500); since JD2433500 - see Table.
DH    Peg    P var. Max = 2414981.537 + 0.25550478d*E
             (JD2414000 - 24000) [01158];
             Max = 2427695.390 + 0.2555107d*E (JD2424000 - 33500)
             [09590]; since JD2433500 - see Table. [Fe/H] = -0.9.
DI    Peg    Min II 9.59. P var. Min I = 2425644.315 + 0.7118144d*E
             (JD2425500 - 30000) [02431]; Min I = 2437559.4096 +
             0.7118182d*E (JD2430000 - 40000) [09592]; Min I =
             2440159.6796 + 0.71181417d*E (JD2440000 - 44500);
             since JD2444500 - see Table.
DK    Peg    d = 0.04P. P var. Min = 2427745.388 + 1.631801d*E
             (JD2427700 - 33700); since JD2433700 - see Table.
DM    Peg    d = 0.03P; Min II 11.0.
DN    Peg    Mean brightness varies with cycles 800 - 1400d and
             A = 0.2m - 0.4m.
DO    Peg    P var. Min = 2434272.350 + 2.61394d*E (JD2428000 - 34700)
             [00485]; since JD2434700 - see Table.
DV    Peg    Min II 12.1.
DY    Peg    P var. Max = 2432751.9624 + 0.072926372d*E
             (JD2429000 - 38000); since JD2438000 - see Table.
             The basic pulsation is superimposed by the secondary one
             with P1 = 0.05570d [09594]. A var, M - m var (Pi = 0.2358d):
             0.55m < A < 0.67m, 0.24P < M - m < 0.42P. Delta(S) = 6.
DZ    Peg    P var. Max = 2429127.211 + 0.6073407d*E
             (JD2419000 - 28800); Max = 2429127.189 + 0.6073761d*E
             (JD2429100 - 33500); since JD2433500 - see Table.
EE    Peg    Min II 7.06. The third body (Porb = 1464d, T0 = 2443120).
EF    Peg    VB B (A 14.0m; B 5", 305deg).
EH    Peg    d = 0.08P.
EQ    PegA   VB A (B = EQb Peg; A = 6.87", Porb = 359 yr, E = 0.20.
             [09597]); mu = 0.560", P = 91.7deg. A (B) >= 1.4m.
EQ    PegB   VB B (A = EQa Peg). a = 6.87'' P orb = 1464d,
             T0 = 2443120. A(U) >= 1.9m.
ET    Peg    Delta(S) = 4.
EU    Peg    Min II 12.3.
EZ    Peg    On 1943 November 16 the spectrum of the star was B [02875];
             probably at that time the star had a flare.
FL    Peg    Min II 14.0.
FU    Peg    Blazhko effect (Pi = 150d); A var;
             15.2m <= Max <= 15.8m; 0.15P <= M - m <= 0.50P.
GH    Peg    Depth of Min II 0.13m.
GR    Peg    P var. Max = 2436492 + 69.93d*E (JD2436420 - 38740);
             since JD2440470 - see Table.
GT    Peg    mu = 0.51", P = 96deg. Epoch of the light minimum is given.
             During the flares A(U) < 3.6m.
GV    Peg    Delta(S) = 5:.
GW    Peg    Min II 15.1.
GX    Peg    SB1 (Porb = 2.340939d [06103]).
GZ    Peg    VB A (B 10.6m, A3V, 32.7", 198deg).
HN    Peg    [Fe/H] = -0.09. Epoch of light minimum is given.
             The variability of emission in H and K call lines with
             P = 4.63d was detected [09600].
HP    Peg    Vr = -381 km/s.
HR    Peg    S4+/1+ .
HZ    Peg    Min II 17.6.
II    Peg    mu = 0.575", p = 86.5deg. SB1
             (T0 = 2443030.396 + 6.724464d*E); T0 is the epoch of the
             inferior conjunction of K-star. The epoch of the
             distortion wave maximum is given in the Table. Mean
             brightness of the system varies.
IK    Peg    SB1 (Porb = 21.724d). Multiperiodicity [09609].
IM    Peg    SB1 (Porb = 24.649d).
QQ    Peg    Variability needs confirmation.
V0341 Peg    SB, Porb = 2.1779d.
V0342 Peg    Suspected SB.
bet   Peg    VB A (B 11.2m, 109", 211deg).
eps   Peg    VB A (B 12.66m, 81", 325deg; C 8.65m, 140", 321deg).
             Usually varies in the range 2.29m - 2.44m V. On 1972
             september 26/27 in the interval 23h58m - 00h02m UT it was
             bright (0.7m V), then at 00h09m UT decreased to 2.4m V
             [06875]. On 1847 November 5 the star was 3.5m, then the
             brightness increased but on November 6 it was still
             fainter than normal [09606].
tau   Peg    P2 = 0.04895d; PB = 0.4943d.
S     Per    In the region of the open cluster h, khi Per.
             OH, H2O, SiO maser.
             In 1920 - 1969 there were secondary
             waves with cycles of 300d - 700d and Delta(m) ~1m [08630];
             in 1935 - 1961 P1 = 807d, P2 = 930d [09694].
T     Per    Other periodicities were noted. In the region
             of open cluster h, khi Per.
U     Per    P var. Max = 2411683 + 316.10d*E (before JD2422500);
             Max = 2422748 + 326.53d*E (JD2422500 - 34000);
             since JD2434000 - see Table.
V     Per    VB A (B 14m, 28", 278deg).
W     Per    P2 = 2667d +- 460d is superimposed.
X     Per    3U 0352 + 30. LX/Lopt = 10**(-2). ADS 2859 A (B =
             V397 Per, M3III, 22.5", 12deg). SB.
             IR excess. X-ray pulsar (P = 13.93m).
             Further periodicities were noticed in X-ray, optical,
             spectroscopic observations: 22.4h, 308.33d, 580.7d.
Y     Per    P var. Max = 2414990 + 254.74d*E (JD2415000 - 18000);
             Max = 2418049 + 246.25d*E (JD2418000 - 22000);
             Max = 2422242 + 253.62d*E (JD2422000 - 41000);
             since JD2441000 - see Table.
Z     Per    d = 0.028P; Min II 9.8.
             P var. Min = 2418173.663 + 3.056422d*E (JD2415000 -
             19000) [01961]; Min = 2425481.416 + 3.05636d*E
             (JD2419000 - 31000) [00978]; since JD2431000 - see Table.
RR    Per    P var. Max = 2424280 + 392.01d*E (JD2416000 - 28500);
             since JD2428500 - see Table.
RS    Per    In the region of the open cluster h, khi Per.
             According to [01053], P = 152d.
RT    Per    Min II 10.67. P var. Min = 2411963.2995 + 0.84941322d*E
             (JD2411317 - 19400); Min = 2419702.3124 + 0.84940248d*E
             (JD2419400 - 29300); Min = 2429751.6066 + 0.84941274d*E
             (JD2429300 - 33000); since JD2433000 - see Table.
RV    Per    Min II 10.4. P var. Min = 2417972.345 + 1.973489d*E
             (JD2417000 - 25500); since JD2432500 - see Table.
RW    Per    The light curve shape var,
             d = 0.03P - 0.000P. Min II 9.78. P var. Before
             JD2425720 Min = 2425720.0185 + 13.198910d*E;
             Min = 2429217.5946 + 13.198399d*E (JD2425720 - 36700);
             since JD2436700 - see Table.
RY    Per    d = 0.014P; Min II 8.65.
RZ    Per    S 3/7 e. P var. Before JD2430500 Max = 2415034 + 353.19d*E;
             since JD2430500 - see Table.
ST    Per    VB A (B 12.1m, 11.6", 6deg, 1928). d = 0.014P, Min II 9.62.
             P var. Min = 2419030.5038 + 2.6483615d*E
             (JD2418500 - 27000) [09740]; Min = 2429528.5897 +
             2.6483488d*E (JD2427000 - 34600) [02389]; Min =
             2439091.716 + 2.648353d*E (JD2439000 - 42400);
             since JD2442400 - see Table.
SU    Per    In the region of the open cluster h, khi Per.
SV    Per    [A/H] = 0.6. SB2, hot companion.
             P var? Before JD2435000 Max = 2419055.145 +
             11.12875d*E [02431]; since JD2435000 - see Table.
SX    Per    [A/H] = 0. The chart in [08300]
SY    Per    In the region of the open cluster NGC 1528.
TU    Per    Delta(m), P var. Before JD2427200 Max = 2418572.288 +
             0.6070775d*E; Max = 2427119.334 + 0.6070643d*E
             (JD2427200 - 36000); since JD2436000 - see Table.
TV    Per    P2 = 1080d is superimposed.
TX    Per    [Fe/H] = -0.88. OH maser.
TZ    Per    VB A (B14m, 13", 290deg). Mu alpha = +0.012",
             mu delta = -0.050". In the region of the open
             cluster h, khi Per.
UX    Per    [A/H] = -0.3.
UY    Per    [A/H] = -0.3. In the region of the open clusters King 4,
             Czernik 8.
UZ    Per    P2 = 91d is superimposed.
VV    Per    Twice shorter P is possible [00960].
VX    Per    In the region of the open cluster h, khi Per.
             [A/H] = -0.2. P var. Since JD2431000 - see Table.
VY    Per    In the region of the open cluster h, khi Per.
             [A/H] = -0.3.
VZ    Per    VB A (B 16.9m pg, 17", 180deg). In the region of the open
             cluster Tr 2.
WY    Per    P var. Min = 2425234.460 + 3.327126d*E (JD2421500 - 26000)
             [01072]; since JD2441500 - see Table.
XX    Per    VB A (B 9.7m vis, 21", 176deg, 1909).
             Mean brightness var, P = 4100d.
XY    Per    ADS 2788 AB (delta(mV) = 0.6m - 2.5m, 1.4", 75deg,
             SpA = A2II, SpB = B6e). IR excess.
XZ    Per    Min II 11.6. P var? Min = 2425150.439 + 1.1516282d*E
             (JD2425000 - 29000) [00522]; Min = 2437932.411 +
             1.1516347d*E + 0.005d*sin(0.09091deg*E) (JD2432000 -
             38000) [00001]; since JD2438000 - see Table.
YZ    Per    In the region of the open cluster h, khi Per.
ZZ    Per    The coordinates are possibly erroneous.
AB    Per    d = 0.045P; Min II 10.5. VB (Delta(m) = 0.0m vis, 0.20",
             86.4deg, 1978).
AD    Per    Mean brightness var, P = 2950d.
             In the region of the open cluster h, khi Per.
AE    Per    P2 = 2150d is superimposed.
AG    Per    ADS 2990 A (B Delta(m) = 2.0m, 0.9", 225deg, 1975; C 12.6m,
             36", 118deg, 1948). The combined brightness AB is given.
             Min II 7.00, DII = 0.10P, dII = 0. Apsidal motion:
             Min II - Min I = 1.01435d + 0.0884d*sin(0.0278deg*E +
             49.1deg).
AR    Per    P var, nonlinear term: +1.18d*10**(-11)*E**2.
             [Fe/H] = -0.17.
AS    Per    Delta(m) var, d (Delta(B))/dt = -0.01m/yr.
AV    Per    P = 250 - 300d.
AW    Per    SB2, companion B6V, Delta(m) (companion - AW) = 2.8m vis.
AX    Per    Epoch of Min is given. The variability with Delta(m) up to
             0.7m pg is caused probably by the orbital motion. Outburst
             activity is superimposed.
AY    Per    d = 0.009P.
BE    Per    In the region of the open cluster CR 39.
BI    Per    In the region of the open cluster Berk 9.
BL    Per    P = 125 - 130d.
BM    Per    [Fe/H] = -0.04.
BP    Per    Min II = Min I. In the region of the open cluster
             Cr 39.
BU    Per    Max brightness var, P = 8.1yr [01085]. In the region of
             the open cluster h, khi Per.
CC    Per    Min II 14.1.
CI    Per    P var (3.35d - 3.40d), possibly with a period of 4000d.
             The light curve shape var.
CK    Per    d = 0.05P:.
CM    Per    d = 0.052P. In the region of the open cluster Stock 2.
CO    Per    In the region of the open cluster Stock 2.
CR    Per    Elements need confirmation. In the region of the open
             cluster Stock 2.
CS    Per    In the region of the open cluster Stock 2.
CZ    Per    In the region of the open cluster h, khi Per.
DE    Per    d = 0.01P?
DF    Per    In the region of the open cluster h, khi Per.
DG    Per    d = 0.021P.
DK    Per    The depth of Min II 0.05m. In the region of the open
             cluster h, khi Per.
DM    Per    Min II 8.02, DII = 0.17P.
             Depths of Minima, the shape of Min II var.
             In the region of the open cluster h, khi Per.
DO    Per    In the region of the open cluster h, khi Per.
DP    Per    In the region of the open cluster h, khi Per.
DR    Per    In the region of the open cluster h, khi Per.
DS    Per    In the region of the open cluster h, khi Per.
DT    Per    In the region of the open cluster h, khi Per.
DU    Per    In the region of the open cluster h, khi Per.
DV    Per    Min II 14.5.
DY    Per    In the region of the open cluster Tr 2.
DZ    Per    Min II 14.7. In the region of the open cluster Tr 2.
EL    Per    Before JD2428900 Max = 2427980 + 167d*E;
             during JD2428900 - 31000 - see Table.
EO    Per    IR excess?
ER    Per    Mean brightness var, P ~900d.
EU    Per    Min brightness var, P ~900d.
EW    Per    Superimposed waves 70d - 180d.
             In the region of the open cluster Stock 4.
EX    Per    Min II 12.5.
FM    Per    VB A (B 12.1m, 3", 285deg). P var? Max = 2429982.268 +
             0.489199d*E (JD2428000 - 30600);
             During JD2433700 - 36000 - see Table.
FR    Per    In the region of the open cluster NGC 1528.
FV    Per    Cycles 300 - 350d, 1800d:.
FX    Per    d = 0.04P. In the region of the open cluster NGC 1582.
FY    Per    Possible periods 0.0702d, 0.4407d.
             Photometric spectral type B1V.
FZ    Per    In the region of the open cluster h, khi Per.
GH    Per    P = 220d is possible.
GK    Per    SB2 (sdBE + K2IVp).
             The following types of activity are being observed after
             the return to the normal brightness: rapid irregular
             variations (Delta(m) ~0.1m in several minutes); irregular
             fluctuations from night to night (Delta(m) up to 0.3m);
             slow irregular variations (Delta(m) = 1.5m in several
             dozen days); bursts with light increase in 10d - 30d and
             decrease in 10d - 40d, Delta(m) up to 3.5m, the mean
             interval between bursts being delta(t) = 820d [09686, 09788].
             According to [10198], the radial velocities are
             represented with the elements Max (Vr > 0) = 2444912.966 +
             1.996803d*E (Kabs = 124 km/s, Kem = 34 km/s). According
             to [10199], the 2d variation is modulated with a period
             of 0.131623d, Max (delta(Vr)) ~2443787.995 (Kabs =
             15 km/s, Kem = 20 km/s). During a burst the sinusoidal
             modulation of X-ray flux was recorded,
             Tmax = 24455555.67456 + 0.004066443d*E [09786].
             ExpAnding envelope (0.454"/yr, 1948 - 1964;
             0.432"/yr, 1964 - 1981, [09787]).
GP    Per    [A/H] = -0.5.
GQ    Per    According to [00021], Sp K0.
HQ    Per    [A/H] = -0.3.
HS    Per    In the region of the open cluster Stock 4.
HV    Per    d ~0.03P.
HW    Per    Min II 13.3. Min II - Min I = 0.45P:.
HY    Per    Three of the four min in [01079] are not satisfied with the
             elements.
HZ    Per    [A/H] = -0.8. B_V: +1.93, +2.34.
II    Per    Min II 13.6. In the region of the open cluster NGC 1582.
IK    Per    Min II 11.6.
IM    Per    Min II 12.7. The elements need confirmation. In the region
             of the open cluster Cr 39.
IO    Per    H2O maser.
IP    Per    IR excess.
IQ    Per    dI = 0.02P. Min II 7.88, DII = 0.12P, dII = 0.03P,
             Min II - Min I = 0.53P. P var? VB A (B = BD + 47deg 921,
             9.30m, A0V np:, 39.3", 175deg); SB1.
IT    Per    dI = 0.06P. Min II 10.0, DII = 0.24P:, dII = 0.16P:.
             VB (Delta(m) = 1.7m, 12", 37deg).
             The range of the combined brightness is given.
IW    Per    SB1. Min II 5.83.
IX    Per    The depth of Min II 0.02m.
             VB A (B 10.6m, 5", 208deg).
IZ    Per    Min II 8.3.
KK    Per    In the region of the open cluster h, khi Per.
KP    Per    Beat phenomenon: P1 - see Table,
             A1 = 0.0323m B; P2 = 0.1980855d, A2 = 0.0235M B; P3 =
             0.2270986d, A3 = 0.0072M B.
KR    Per    Min II 11.1.
KS    Per    SB (Porb = 360.47d).
             The main component is a helium star. Besides the
             semiregular variability (see Table), variations were noted
             with P = 50 - 100 Min and Delta(m) of several hundredths
             of a magnitude. IR excess. Variable polarization (P - 1%).
KT    Per    Quasi-periodic oscillations during outbursts: P =
             22.9s - 29.5s [05959], 82s, 90s, 147s [09791], Delta(m)
             up to ~0.01m.
KV    Per    [Fe/H] = -0.96. P var. Max = 2428950.400 + 0.24942d*E
             (JD2428950 - 29200); since JD2429500 - see Table.
KW    Per    Min II 10.8. P var. Min = 2426295.450 + 0.931255d*E
             (JD2423400 - 39500) [04009]; since JD2440000 - see Table.
KY    Per    In the region of the open cluster h, khi Per.
KZ    Per    In the region of the open cluster h, khi Per.
LL    Per    In the region of the open cluster h, khi Per.
LM    Per    In the region of the open cluster h, khi Per.
LN    Per    In the region of the open cluster h, khi Per.
LO    Per    In the region of the open cluster h, khi Per.
LP    Per    In the region of the open cluster h, khi Per.
LQ    Per    In the region of the open cluster h, khi Per.
LR    Per    Very red. In the region of the open cluster h, khi Per.
LX    Per    mu alpha = +0.0065s, mu delta = -0.063". Min II 8.38m.
             DII = 0.05P. Migrating distortion wave:
             P = 475d [09792], Delta(m) up to 0.04m.
MS    Per    Min II 12.1.
MX    Per    IR excess.
NP    Per    Min II 13.0.
NR    Per    P var. Max = 2416780 + 323.0d*E (JD2415750 - 24550);
             Max = 2435060 + 340.2d*E (JD243350 - 35400);
             since JD2436700 - see Table.
NU    Per    A close pair, var is the southern star.
OV    Per    D ~2h.
PP    Per    In the region of the open cluster h, khi Per.
PR    Per    In the region of the open cluster h, khi Per.
QR    Per    Red.
QU    Per    d = 0.03P.
QW    Per    Min II 14.7:.
QX    Per    Min II 16.1.
V0345 Per    In the nebula NGC 1579.
V0346 Per    In the nebula NGC 1579.
V0347 Per    In the nebula NGC 1579.
V0351 Per    In the region of the open cluster h, khi Per.
V0352 Per    In the region of the open cluster h, khi Per.
V0354 Per    In the region of the open cluster h, khi Per.
V0355 Per    In the region of the open cluster h, khi Per.
V0356 Per    In the region of the open cluster h, khi Per.
V0357 Per    In the region of the open cluster h, khi Per. P = 0.21955d
             is possible.
V0358 Per    In the region of the open cluster h, khi Per.
V0359 Per    In the region of the open cluster h, khi Per.
V0360 Per    In the region of the open cluster h, khi Per.
             Other possible periods: 0.40036d, 0.40154d.
V0361 Per    In the region of the open cluster h, khi Per.
V0363 Per    Red.
V0364 Per    Min II 15.6, Max II 14.8.
V0365 Per    Min II 14.3:.
V0376 Per    P2 = 0.09165d, A2 = 0.016m; P1 - see Table,
             A1 = 0.037m. A var.
V0380 Per    SB (Porb = 26d?). The epoch of Min light is given.
V0382 Per    In the region of the open cluster h, khi Per.
V0392 Per    The southern component of a very close pair.
V0394 Per    H2O maser.
V0395 Per    VB A (B 3.5", 90deg).
V0396 Per    In the region of the open cluster alpha Per.
             Observations are also satisfied by P ~1.678d. According
             to [07586], P = 2.4928d or 1.6857d.
V0397 Per    ADS 2859 B (A = X Per; B 22.5", 12deg).
V0398 Per    IN type is also possible.
V0403 Per    In the region of the open cluster h, khi Per.
V0409 Per    Epoch of Min is given.
V0423 Per    ADS 2433 A (B 11.9m, 30.8", 99.2deg); SB.
             Porb is given.
V0424 Per    In the region of the open cluster h, khi Per. IR excess.
V0425 Per    VB A(B 12.8m, 3.6", C 14.3m, 6.8"). In the region of
             the open cluster h, khi Per.
V0428 Per    According to [08639], type IS?
V0432 Per    Min II 11.6.
V0434 Per    Min II 14.9.
V0436 Per    Min II 5.74; Min II - Min I = 0.413P; D II = 0.03P.
V0437 Per    In the region of the open cluster NGC 744.
V0438 Per    In the region of the open cluster h, khi Per. VB (8.7m,
             10.9m, 1".2, 26deg).
             Min II 8.34. The range of combined brightness
             variation is given. The bright component is
             considered to be variable. This suggestion
             needs verification.
V0439 Per    In the region of the open cluster h, khi Per.
V0440 Per    In the region of the open cluster h, khi Per. ADS 1820
             A (B 14.5m, 8".3, 122deg).
V0449 Per    Min II 13.3.
V0451 Per    Min II 15.8.
V0459 Per    In the alpha Per cluster.
V0461 Per    In the alpha Per cluster.
V0462 Per    Min II 14.0.
V0465 Per    P2 = 0.030d is superimposed.
V0466 Per    Superposition of P1 = 5300d +- 250d, P2 = 475d +- 35d
             (Delta(m) = 1.1m), P3 = 0.26d (Delta(m) = 0.5).
V0468 Per    P1 = 925s, P2 = 1022s. mu = 0".29, p = 170deg.
V0469 Per    Changes of line profiles with periods 0.150d, 0.188d,
             0.304d, 0.476d, 0.608d, 1.88d [09814].
             In 1978/1979 non-radial pulsations were observed:
             P1 = 1.74d. P2 = 2.04d [04173, 04180].
V0470 Per    VB A (B 18.8m B, 1" - 2").
V0471 Per    The central star of the planetary nebula M1-2 = VV8.
             According to [09815, 09816], const.
V0547 Per    High proper motion (LTT 10610) not confirmed by HIPPARCOS data.
V0580 Per    The variability may be due to the fainter (B) component.
V0582 Per    A single deep minimum at the bottom of the small-amplitude
             (5.63 - 5.64) wave.
V0592 Per    VB (0".2, 197 deg, 1989.7).
bet   Per    Multiple system (Eclipsing pair = Algol AB; Algol C 4.7m,
             Am, a = 0".10, Porb = 1.862a); Algol AB = ADS 2362 A
             (B 12.7m, 57".5, 156deg, 1920). P var. P = 2.8673442d
             (1784 - 1835); P = 2.8673012d (1835 - 1854);
             P = 2.8672775d
             (1854 - 1901); P = 2.8672967d (1901 - 1913);
             P = 2.8672506d
             (1913 - 1915) [06156]; Min I = 2424477.806 + 2.86730236d*E
             (JD2420500 - 25000); Min = 2425917.203 + 2.86732697d*E
             (JD2425000 - 277000); Min I = 2433194.454 + 2.86731667d*E
             (JD2427700 - 33600); Min I = 2433928.4944 + 2.86732442d*E
             (JD2433600 - 37000); Min I = 2437598.6766 + 2.86733732d*E
             (JD2437000 - 42200); since JD2442200 - see Table.
             Porb (Algol C) = 1.862a may be traced in the deviations;
             a period of 32a may also be real. Depth of Min I var.
             Variable polarization, changes in hydrogen line profiles,
             sometimes emissions in the spectrum. Radio source with
             frequent burst of different amplitude, faint X-ray source.
del   Per    Variable emission lambda 1650 A [06905]. Vr var,
             A = 16 km/s.
ksi   Per    In the far IR range (lambda = 10 mkm) Delta(m) > 1m. In
             the far IR range (lambda = 10 mkm ) Delta(m) > 1m; the
             variability is related to mass loss.
omi   Per    VB A (B 8.4m, 0.96'', 29.7deg,1972). Possible
             superposition of BCEP type oscilations.
rho   Per    A slower variation of the mean light is possible.
             mu alpha = 0.0111s, mu delta = -0.102''.
phi   Per    SB2. (Porb = 126.696d). v*sin(i) = 450km/s. A var (P ~Porb).
b     Per    SB2. Depths of minima differ by 0.03m. Third body? ,
             P = 701d. Radio source. In  the region of the open cluster
             NGC 1545.
R     Phe    P var. Max = 2405121 + 271.0d*E(JD2405000 - 11500);
             Max = 2414570 + 266.26d*E(JD2414500 - 25500);
             since JD2425500 - see Table.
T     Phe    P var. Max = 2411252 + 281.00d*E(JD2410000 - 30000);
             since JD2430000 - see Table.
W     Phe    P var. Max = 2414960 + 328.65d*E(JD2414500 - 19500);
             Max = 2424530 + 332.87d*E(JD2424500 - 30200);
             since JD2436000 - see Table.
RS    Phe    P var?
RT    Phe    P = 208d?
RV    Phe    P var?; (k-b)2 = 0.06; Delta(S) = 8:
SX    Phe    mu = 0.894", ro = 163.1deg. P var. Max = 2433923.9618 +
             0.054964519d*E1 - 0.00337d*sin(2pi*(0.28503379*E1 + 0.074))
             (JD2433900 - 36900); since JD2436900 - see Table.
             There is a periodic term in the elements given in the
             Table: -0.00325*sin(2pi*(0.28503575*E2 - 0.107)). According
             to [09614] for epoch 1950.0 P0 = 0.054964509,
             P1 = 0.042772831, Pb = 0.1928355; dP0/dt = -87*10**(-13),
             dP1/dt = -174*10**(-13), dPb/dt = 2.46*10**(-10).
             P1/P0 = 0.778; 0.8m <= A <= 0.3m;
             0.2p <= M-m <= 0.4p. [Fe/H] = -0.6.
WW    Phe    Min II 12.7.
YZ    Phe    Min II 13.0.
AD    Phe    Min II 10.80. P var. Min I = 2436847.375 + 0.3799277*E
             (JD2428650 - 36850); since JD2436850 - see Table.
AE    Phe    Min II 8.19; 0.033p <= dI <= 0.05p; dII = 0.00.  The
             shape of the light curve varies with periods 55.9d and
             95.3d [09615]. P var. Min I = 2440857.8140 + 0.36237459*E
             (JD2438250 - 40870) [07388]; Min I = 2441969.57074 +
             0.36237186d*E (JD2440870 - 42000) [09616]; Min I =
             2442654.8201 + 0.3623741d*E (JD2441950 - 42660) [09533];
             since JD2443700 - see Table.
AG    Phe    Min II 8.95. P var. Min I = 2440415.231 + 0.7553429d*E
             (JD243800 - 40850); since JD2443750 - see Table.
AI    Phe    Min II 8.89; dI = 0.0035; Min II - Min I = 0.46p.
AU    Phe    Min II 13.0. According to [09517] the P value given in
             the Table is wrong.
AX    Phe    mu = 0.234", p = 70deg. Multiperiodical: P i = 606.8s,
             682.7s, 744.7s, 840.2s (Ai ~0.01m).
CG    Phe    Type RRC: is also possible.
gam   Phe    SB1 (P orb = 193.85d).
zet   Phe    VB A (B 7.0m, A7:, 0.46", 51.4deg, 1965.9; C 8.0m,
             F7V, 6.4"). Total light range of A and B components is
             given in the Table. Min II 4.22, MinII - MinI = 0.507p;
             dII = 0.02p.
iot   Phe    VB A (B 12.7m, 7.7", 270deg).
ksi   Phe    VB A (B 12.1m, 13.2", 253deg). Epoch of MinI(v) is given
             in the Table. A(v) = 0.13m.
rho   Phe    Frequency analysis results see also in [09619, 09620, 9621].
psi   Phe    SB.
R     Pic    P var. Max = 2413413  +  165.8d*E (JD2413000 - 23600);
             since JD2423600 - see Table. Light curve (1923 - 1953)
             [01054].
S     Pic    P var. Max = 2413595  +  424.7d*E (JD2405500 - 23000);
             since JD2423000 - see Table. OH emission.
U     Pic    P var. Max = 2428103.565  +  0.44036450*E (JD2414000 -
             29000) [00353]; since JD2438400 - see Table. (k - b)2 =
             0.17; Delta(S) = 3.
X     Pic    Min II 10.8
RR    Pic    Since 1965 periodic light variations were detected
             with A(B) = 0.33m and elements Max = 2438815.380 +
             0.14502545d*E. These variations are superimposed by
             others with A(B) = 0.036m and period ~15.6 min or
             15.4 min [09612]. There are also rapid oscillations
             with periods in the range 20 - 40s [09613].
RT    Pic    Not seen only on one plate; defect?
RV    Pic    Min II 9.79.
SU    Pic    Min II 10.4.
VW    Pic    Variability may be due to component B.
VZ    Pic    Kapteyn's star.
del   Pic    Min II 4.83.
R     Psc    P var. Max = 2418070 + 344.14d*E (JD2397070 - 27700);
             Max = 2432866 + 347.1d*E(JD2427300 - 33000) - see Table.
S     Psc    P var. Max = 2406665 + 405.6d*E (JD2398944 - 2407100);
             Max = 2415930 + 402.6d*E (JD2407100 - 16500); Max =
             2421295 + 413.7d*E (JD2416500 - 21500) - see Table.
U     Psc    P var. Max = 2417230 + 172.71d*E (JD2407720 - 18000);
             Max = 2423840 + 174.3d*E (JD2418000 - 24000) [00001];
             Max = 2424527 + 170.3d*E (JD2423000 - 26100) [00960];
             Max = 2432514 + 174.05d*E (JD2425000 - 33000) [00001];
             since JD2433000 - see Table.
V     Psc    mu alpha = 0.0112s, mu delta = -0.215".
W     Psc    P var. Max = 2412690 + 189.08d*E (JD2412692 - 27100)
             [01193];
             since JD2435000 - see Table.
X     Psc    P var. Max = 2433474 + 357.3*E (JD24295000 - 38000); since
             JD2438000 - see Table.
Y     Psc    P var. Min = 2410002.844 + 3.76582d*E (JD2410000 - 19700)
             [09707]; Min = 2425495.522 + 3.765903d*E
             (JD2423200 - 6300) [01072]; Min = 2430613.384 +
             3.7658895d*E
             (JD2427300 - 30620); Min = 2432865.357 + 3.7658405d*E
             (JD2430620 - 32900); Min = 2435693.452 + 3.7657765d*E
             (JD2432860 - 36600) [00001]; Min = 2441225.473 +
             3.765859d*E
             (JD2439000 - 42500) [06956]; Min = 2443142.29056 +
             3.7658491d*E (JD2442500 - 44000) [08593]; since JD2444000 -
             see Table.
RS    Psc    In the region of the galaxy NGC 251.
RT    Psc    Mean brightness varies with P2 = 533d. According to [08643]
             30d <= P1 <= 70d.
RU    Psc    [Fe/H] = -1.65. P var. [00752, 09714] Max = 2415407.609 +
             0.3903008d*E (JD2414400 - 15700); Max = 2416022.660 +
             0.3902139d*E (JD2415700 - 16600); Max = 2417244.537 +
             0.3902878d*E (JD2416600 - 19200); Max = 2419936.853 +
             0.3903520d*E (JD2419200 - 22000); Max = 2425894.778 +
             0.3903016d*E (JD2422000 - 26200); Max = 2426214.829 +
             0.3903546d*E (JD2426200 - 27300); Max = 2427397.519: +
             0.3902216d*E (JD2427300 - 28000); Max = 2428165.524 +
             0.3903535d*E (JD2428000 - 29300); Max = 2429488.868: +
             0.3904577d*E (JD2429300 - 600) [00752]. Max = 2430053.353 +
             0.390202d*E (JD2430000 - 650); Max = 2430935.366 +
             0.390354d*E (JD2430600 - 940); Max = 2431331.307 +
             0.390457d*E (JD2430940 - 31350); Max = 2432119.417 +
             0.390346d*E (JD2431350 - 32120); Max = 2433162.250 +
             0.390283d*E (JD2432100 - 33200); Max = 2433905.311 +
             0.390261d*E (JD2433200 - 33910); Max = 2433905.311 +
             0.390321d*E (JD2433900 - 35430); Max = 2435429.502 +
             0.390412d*E (JD2435420 - 35800); Max = 2435781.265 +
             0.39027d*E (JD2435780 - 36130); Max = 2436501.361 +
             0.39032d*E (JD2436130 - 36510); Max = 2436534.190 +
             0.39043d*E (JD2436500 - 36850); Max = 2436845.351 +
             0.39025d*E (JD2436840 - 37200); Max = 2437181.358 +
             0.39031d*E (JD2437180 - 37610); Max = 2437994.329 +
             0.39026d*E (JD2437610 - 38000); [00001].
             Max = 2438303.950 + 0.39040d*E (JD2438000 - 38400) [03879].
             Max = 2438375.409 + 0.39027d*E (JD2438370 - 38650) [00001].
             Max = 2439435.2421 + 0.390385d*E (JD2438650 - 39500)
             [09713]. Max = 2439435.242 + 0.390313d*E (JD2439430 - 39800);
             Max = 2439771.3049 + 0.39046d*E (JD2439770 - 40140) [00001].
             Since JD2440140 - see Table. According to [03569] A var
             with P = 28.8d.
RV    Psc    Min II 12.0.
RY    Psc    (k-b)2 = 0.03, Delta(S) = 7. P var. Max = 2419677.268 +
             0.52971027d*E (JD2414000 - 22000); Max = 2425148.192 +
             0.52972643d*E (JD2422000 - 25500) [01337]; Max =
             2425508.390 + 0.5297291d*E (JD2425500 - 40000);
             Max = 2441538.476 + 0.52972911d*E (JD2441000 - 41650)
             [07984]; since JD2442660 - see Table.
RZ    Psc    Algol-like.
SS    Psc    (k-b)2 = 0.19; Delta(S) = 2. Blazhko effect:
             -0.04d <= O-C <= +0.04d; Min(O-C) = 2437520 + 136d*E
             [09731].
SU    Psc    Min II 11.3.
SW    Psc    P var. Max = 2425177.298 + 0.5212844d*E (JD2419670 -
             25200) [04191]; Max = 2425177.256 + 0.5212642d*E
             (JD2425170 - 38000) [03506]. Since JD2438600 - see Table.
             There is a periodic term in the elements given in the
             Table: + 0.0132d*sin(5.440deg*(E + 2)). Blazhko effect
             (Pi = 34.5d).
SX    Psc    P var. Min = 2427811.357 + 0.825882d*E (JD2425580 - 36000)
             [01218]; Min = 2437202.453 + 0.825877d*E
             (JD2436000 - 39900)
             [00001]; since JD2439800 - see Table.
SZ    Psc    Min II 7.38. P var.
             There is a square term in the elements given in the Table:
             -0.113d*10**(-6)*E**2.
TY    Psc    Porb = 0.080d [09735].
             The cycle of supermaxima is 370d [09675].
UU    Psc    VB A (B 7.60m, F4V, 11.5", 148deg, 1966.9). Min II 6.04;
             Min II - Min I = 0.55P.
             Elliptical orbit and rotation of the line of apsides are
             possible.
UV    Psc    Min II 9.54. P var. Min I = 2424134.574 + 0.8610475d*E
             (JD2414600 - 24150) [00001]; Min I = 2428038.555 +
             0.861046d*E (JD2424150 - 36700) [02924];
             since JD2436700 - see Table. The shape of the light
             curve varies.
UW    Psc    Min II 11.0:.
UZ    Psc    SB1 (Porb > 1 yr [05751]).
VZ    Psc    Mu = 0.43", P =  65deg. Min II 10.43.
WW    Psc    VB A (B 13.1m, 31").
WX    Psc    OH, H2O, SiO maser.
ZZ    Psc    P1 = 612s, P2 = 816s [07476].
             Nonradial modes [08467].
AG    Psc    P (Vr) = 0.055d.
AH    Psc    The star was seen in 1854 - 60; since 1862 it was not
             observed.
AO    Psc    Epoch of Max brightness is given. Light variations with
             Porb = 0.1496263d are superimposed by variations with
             P = 858.6861s and twice smaller amplitude (Max =
             2444815.00276 + 0.009938496d*E; M-m = 0.54P), and
             also by still smaller oscillations with P = 805.2059s
             (Max = 2444815.00294 + 0.009319513d*E). The last period
             is the X-ray impulse period which is equal to
             the period of rotation of the compact object (probably
             a white dwarf).
R     PsA    P var. Max = 2417385 + 293.00d*E (JD2405000 - 26000);
             Max = 2432896 + 291.50d*E (JD2426000 - 38000);
             since JD2438000 - see Table.
S     PsA    P var. Max = 2417853 + 271.0d*E (JD2411000 - 18000);
             Max = 2426880 + 273.6d (JD2418000 - 27000); Max =
             2434714 + 270.3d (JD2427000 - 35000); since
             JD2434000 - see Table.
X     PsA    Min II 14.2.
RW    PsA    Min II 11.63.
TX    PsA    VB B (A 13.0m pg; B 37", 131deg); mu = 0.22", p = 117deg.
pi    PsA    SB (Porb = 178.3177d [05769]).
R     Pup    In the region of the open cluster NGC 2439.
U     Pup    P var. Max = 2415090 + 314.26d*E (JD2408000 - 22800);
             since JD2422800 - see Table.
V     Pup    VB A (B 10.0m, 7", 0, 70deg; C 11.0m, 19.0", 48deg).
             Min II 4.82. P var. IO - CI < 0.02d.
W     Pup    P var. Max = 2420990 + 120.68d*E (JD2412500 - 23600);
             Max = 2424725 + 119.9d*E (JD2423600 - 26300);
             Max = 2432200 + 120.68d*E (JD2426300 - 40800);
             since JD2440800 - see Table.
X     Pup    P var. Max = 2414889.8 + 25.939d*E (JD2408800 - 16000);
             Max = 2435188.76 + 25.9610d*E (JD2419000 - 35190)
             [02392]; Max = 2436279.50 + 25.97d*E
             (2435190 - 38000) [00001]; since JD2438000 - see Table.
Z     Pup    OH, H2O, SiO emission.
             P var. Max = 2424256 + 513.90d*E (JD2413900 - 24500);
             since JD2424500 - see Table.
RS    Pup    Surrounded by the reflecting nebulosity with a radius of
             1.4' [09634]. P var. Max = 2419186.3 + 41.337d*E
             (JD2414000 - 24000) [02049]; Max = 2427083.613 + 41.414d*E
             (JD2425800 - 28300) [02440]; Max = 2434823.23 + 41.38535d*E
             (JD2433750 - 34900) [09636]; since JD2435700 - see Table.
RW    Pup    P var. Max = 2430175 + 332.5d*E (JD2424500 - 30200)
             [00001]; since JD2435800 - see Table.
RX    Pup    Light curve (1890 - 1925) [01265].
             Mira type component light variations are observed in the
             infrared region of spectrum: Max = 2444530 + 580d*E,
             3.99m - 6.00m J, M - m = 0.50P [09518].
ST    Pup    [A/H] = -0.9.
             The light curve shape and the period vary strongly:
             0.10P < M - m < 0.30P; 17.4d < P < 19.19d.
             P = 19.188d (JD2415000 - 17000); 18.949d
             (JD2417000 - 18000), 18.8065d (JD2418000 - 19000),
             18.721d (JD2419000 - 20000), 18.714d (JD2420000 - 21000),
             18.717d (JD2421000 - 22000), 18.6175d (JD2422000 - 23000),
             18.678d (JD2423000 - 24000), 18.735d (JD2424000 - 25000),
             18.796d (JD2425000 - 26000), 18.817d (JD2426000 - 27000)
             [01266]. Max = 2427779.6 + 18.846d*E (JD2427000 - 28000)
             [01266]; Max = 2428893.9 + 18.885d*E (JD2428000 - 29000)
             [00016]; Max = 2429697.51 + 19.188d*E (JD2429000 - 30000)
             [01266]. P = 19.142d (JD2430000 - 31000),
             19.145d (JD2431000 - 32000) [01266].
             Max = 2435395.430 + 18.559d*E (JD2435160 - 500)
             [06006]; Max = 2435617.45 + 18.8864d*E (JD2435500 - 5620)
             [02309]; Max = 243957.3 + 17.4d*E (JD2438700 - 39600)
             [06611]; since JD2444000 - see Table.
SV    Pup    P var. Max = 2419010 + 166.6d*E (JD2413660 - 18000);
             Max = 2423090 + 169.8d*E (JD2418000 - 23100);
             Max = 2426782 + 167.8d*E (JD2423100 - 27500);
             since JD2427500 - see Table.
SW    Pup    Min II 9.1; d = 0.029P.
TT    Pup    Min II 13.6.
TY    Pup    Min II 8.87.
UZ    Pup    Min II 10.0.
VV    Pup    mu = 0.100", P = 165.0deg.
             The epoch of light maximum is given. The mean
             brightness varies by 2 - 3m. Intervals of active light
             variation with amplitude up to 2m during maximal mean
             brightness are observed. During low activity intervals
             when amplitude is about 0.3m mean brightness is minimal;
             during this time the ellipsoidal light variations of the
             system are observed in the range 15.1m - 15.3m J with the
             elements Min = 2427889.6509 + 0.0697468256d*E [09644].
             The white dwarf rotation period is equal to the orbital
             period. There are flickerings. Spectrum description
             [09472, 09645].
VW    Pup    P var. Max = 2425184.67 + 4.28405d*E (JD2422660 - 25600)
             [00973]; Max = 2435554.86 + 4.28519d*E (JD2425600 - 35600)
             [02309]; since JD2435500 - see Table.
VX    Pup    P1 = 2.1389d (A1 = 0.29m); A0 = 0.31m; P1/P0 = 0.71042.
VY    Pup    The depth of Min II 0.04m.
VZ    Pup    [A/H] = -0.3. P var. Max = 2434864.90 + 23.1640d*E
             (JD2426700 - 35300) [02309]; since JD2435300 - see Table.
WW    Pup    P var. Max = 2424497.73 + 5.5159d*E (JD2423520 -
             26000) [00973]; since JD2426000 - see Table.
WX    Pup    P var. Max = 2435042.184 + 8.93825d*E (JD2422000 -
             35100) [02431]; since JD2435000 - see Table.
WZ    Pup    P var. Max = 2427861.33 + 5.02657d*E (JD2421100 -
             29400) [02392]; since JD2429400 - see Table.
XX    Pup    P var. Max = 2426338.503 + 0.51719805d*E
             (JD2426300 - 39500) [03572]; since JD2441700 - see Table.
             (k - b)2 = 0.07. The spectral type according to CA II is
             given.
XY    Pup    Min II 9.4; d = 0.042P.
XZ    Pup    Min II 7.90. P var. Min I = 2440629.7969 + 2.192383d*E
             (JD2425850 - 41700) [00099]; since JD2441700 - see Table.
YY    Pup    The depth of Min II 0.05m.
AE    Pup    In the region of the open cluster Cr 173.
AF    Pup    Min II 13.5.
AG    Pup    Min II 10.9.
AH    Pup    The depth of Min II 0.05m.
AN    Pup    Min II 10.7.
AQ    Pup    VB A (B 11.13m, < 15"; C 12.83m, < 15"). [A/H] = -0.1.
             The range of the variation of combined light is given.
             P var. Max = 2429734.59 + 29.931d*E (JD2427500 - 33000)
             [03474]; Max = 2433296.2 + 30.018d*E (JD2433000 - 35850)
             [02474]; Max = 2436625.9 + 29.8568d*E
             (JD2435850 - 36700) [03601]; Max = 2441760.63 + 30.032d*E
             (JD2436600 - 42700) [09671]; since JD2443400 - see Table.
AR    Pup    The mean brightness varies with P = 1200d.
AS    Pup    In the region of the open cluster NGC 2546. P var.
             Max = 2416110 + 331.4d*E (JD2415460 - 26000); since
             JD2426000 - see Table.
AT    Pup    In the region of the open cluster NGC 2546.
             P var. Max = 2426758.205 + 6.6648d*E (JD2426700 - 35600)
             [02202]; since JD2435600 - see Table.
AU    Pup    Min II 9.28. P var. Min I = 2428111.304 + 1.126418d*E
             (JD2414700 - 28200) [00007]; since JD2439000 - see Table.
AV    Pup    Min II 11.0.
AW    Pup    VB A (B 11.7m, 3.7", 258deg). Period probably must be
             doubled.
AY    Pup    Min II 12.5.
AZ    Pup    Min II 10.1.
BB    Pup    (k - b)2 = 0.24; Delta(S) = 3.
BH    Pup    In the region of the open cluster Cr 173.
BI    Pup    In the region of the open cluster Cr 173.
BK    Pup    In the region of the open cluster Cr 173.
BL    Pup    Min II 14.2.
BN    Pup    In the region of the open cluster NGC 2533.
BP    Pup    Min II 12.3.
BQ    Pup    The shape of the light curve possibly varies.
BR    Pup    Min II 12.9.
BT    Pup    Min II 14.5. In the region of the open cluster NGC 2482.
BU    Pup    Min II 13.9. In the region of the open cluster NGC 2447.
BW    Pup    The depth of Min II 0.15m.
BX    Pup    In the region of the open cluster NGC 2482.
CE    Pup    P var? [07934].
CH    Pup    P var. Max = 2428465 + 491.0d*E (JD2428400 - 37300);
             since JD2437300 - see Table.
CO    Pup    P var? The epoch of light minimum is given.
CP    Pup    In 1981 the radius of the shell expanding with
             Vexp = 710 km/s was equal to 7" [09689, 09559].
CX    Pup    d = 0.05P.
CY    Pup    d = 0.01P:; Min II 13.0.
CZ    Pup    Min II 13.1.
DD    Pup    Min II 14.6; Min II - Min I = 0.572P.
DE    Pup    Min II 12.9.
DF    Pup    Min II 12.8.
DK    Pup    Min II 13.0.
DM    Pup    Min II 13.7; Min II - Min I = 0.62P.
DN    Pup    Min II 13.5.
DO    Pup    Min II 13.3.
DR    Pup    Min II 13.3:.
DS    Pup    Min II 13.4.
DT    Pup    Min II 14.3.
EK    Pup    VB A (B 15", 270deg). P var? Max = 2427747.89 + 2.62587d*E
             (JD2425500 - 29500) [01343]; since JD2434500 - see Table.
EL    Pup    P > 1.3d? In the region of the open cluster NGC 2437.
EN    Pup    Min II 11.4.
EQ    Pup    Min II 10.9.
ES    Pup    According to [00412], Max = 2430377 + 187d*E.
             The elements given in the Table are valid in the interval
             JD2425600 - 29700.
EU    Pup    Min II 14.8.
FK    Pup    A var (P2 = 3000d). Strong SiC2 bands in the spectrum.
FM    Pup    Min II 14.2.
GG    Pup    S5/5.
GH    Pup    VB A (B 10", 195deg; C 16", 280deg; D 14", 315deg). P var.
             Max = 2425450 + 800d*E (JD2425300 - 28000); since
             JD2428700 - see Table. Very red.
GI    Pup    In the region of the open cluster NGC 2437.
GK    Pup    IN the region of the open cluster NGC 2437.
GN    Pup    VB A (B 16.5m, 10", 80deg).
GP    Pup    Min II 13.5.
GU    Pup    Min II 12.2.
GX    Pup    Min II 13.9. In the region of the open cluster Cr 173.
GY    Pup    Min II 12.3.
GZ    Pup    Min II 12.1.
HH    Pup    (k - b)2 = 0.14, Delta(S) = 1.
HI    Pup    Min II 11.0. In the region of the open cluster Cr 173.
HK    Pup    P var. Max = 2425925.732 + 0.7342532d*E
             (JD2425300 - 36600) [04127]; since JD2436600 - see Table.
HM    Pup    There is a shallow Min II.
HP    Pup    P var?
HW    Pup    P var? Max = 2429756.28 + 13.4532d*E (JD2427100 - 33000)
             [03551]; since JD2433000 - see Table.
KQ    Pup    In the open cluster NGC2422. SB2 (Porb = 9752d [03985]).
KT    Pup    Min II 13.4.
KW    Pup    Min II 11.8.
KX    Pup    Min II 13.04; 0.435P (1930) < Min II - Min I < 0.56P (1973)
             [03474, 08094]; e = 0.15. Apsidal motion.
KY    Pup    Min II 11.1.
LN    Pup    Min II 12.9; Min II - Min I = 0.533P.
LO    Pup    Min II 13.9.
LP    Pup    d = 0.03P:.
LT    Pup    Min II 12.6.
MN    Pup    Min II 13.2.
MQ    Pup    Min II 9.39.
MT    Pup    RCB?
MW    Pup    Min II 9.2.
NO    Pup    VB A [BC 7.19m V, 8.1". 124deg (delta(M) = 0.0m, 0.20",
             275deg,
             1976)]. Min II 6.66; Min II - Min I = 0.582P; e = 0.123.
NQ    Pup    S 4.5/2-.
NW    Pup    Porb = 1d.
NX    Pup    Connected with a cometary nebula.
OR    Pup    In the region of the open cluster NGC 2467.
OS    Pup    VB A (B 6.10m, 67.4").
             In the region of the open cluster C 0812-362.
OU    Pup    In the region of the open cluster IC 2391.
OX    Pup    In the region of the open cluster NGC 2451.
PS    Pup    The depth of Min II 0.028m.
PT    Pup    P2 = 0.168377d. A (lambda 1550) = 0.043m;
             0.015m < A(B) < 0.035m.
PU    Pup    VB (5.2m, 5.6m; 0.11", 43.6deg, 1927). Min II 4.74.
PV    Pup    VB B (A 6.1m; B 16.9", 340deg; C 10.5m, 100.4", 228deg).
             Min II 7.31; DII 0.10P; Min II - Min I = 0.47P.
             The light curve shape in Max and Min II varies.
             The deviations DB from the mean curve vary from -0.06m
             to +0.03m with the elements: Max (IDelta(B)I) =
             2440000.027458 + 1.92207d*E or Max (IDelta(B)I) =
             2440000.219470 + 0.48003d*E.
PW    Pup    Min II 9.54; d = 0.095P. In the region of the open
             cluster NGC 2439.
QS    Pup    0.008m <= A(u) <= 0.015m.
QT    Pup    Probably a member of the open cluster NGC 2477.
QU    Pup    P2 = 0.1680d or 0.2019d; 0.010m <= A(u) <= 0.040m.
QV    Pup    May be a member of the open cluster NGC 2489.
V0360 Pup    Type ACV: is also possible.
V0364 Pup    The preceding component of the northern star in the system of two
             CoD-CPD objects, COD-36 3425 and CoD-36 3426 (CPD-36 1171 and CPD-36
             1172).  The cross-identifications of these CoD and CPD objects differ
             from one source to another; our adopted identification is based on the
             paper editions of the catalogs.
V0376 Pup    Type ACV: is also possible.
V0378 Pup    Type BE is also possible.
V0393 Pup    SB, Porb = 2.5248d.
V0419 Pup    Not a nearby star (despite having a Gl number).
omi   Pup    Type EA: is also possible.
rho   Pup    VB A (B 13.7m, 29.6", 15deg). [Fe/H] = +0.13. P var.
             Max = 2435552.807 + 0.14088141d*E (JD2413900 -
             37500) [09756]; Max = 2439887.843 + 0.14088141d*E
             (JD2439800 - 43700); since JD2444000 - see Table.
L   2 Pup    VB A (B 11.5m, 62", 214deg); mu = 0.34", P=18deg. H2O,
             SiO maser.
S     Pyx    P var. Max = 2411770 + 206.60d*E (JD2405500 - 23700);
             Max = 2423765 + 207.0d*E (JD2423700 - 29600);
             since JD2429600 - see Table.
T     Pyx    Previous outbursts were observed in 1890, 1902, 1920, 1944.
RR    Pyx    A close companion 14.5m.
RZ    Pyx    Min II 9.69.
SU    Pyx    d = 0.016P.
TT    Pyx    P = 3.031556d?
TV    Pyx    Depth of Min II 0.05m.
TX    Pyx    Min II 9.8.
TY    Pyx    Min II 7.48.
TZ    Pyx    Min II 11.1.
UZ    Pyx    VB A (B 7.61m, 110", 180deg).
VV    Pyx    VB A (B 8.58m, 0.3").
             Range of the variation of combined light is given.
             Min II 7.03; DII = 0.08P; Min II - Min I =
             0.48P. Min II = 2444622.86709 + 4.5961766d*E.
             Apsidal motion (P = 3200 yr).
VW    Pyx    The nucleus of the planetary nebula K1-2.
             The range of the variations of combined light:
             15.7 - 17.4 pg. The value of P close to
             that found by bond [09767] and the epoch of Max brightness
             are given in the Table.
R     Ret    P var. Max = 2403013 + 280.0d*E (JD2403000 - 13900);
             Max = 2423317 + 276.68d*E (JD2413900 - 25300);
             Max = 2430008 + 279.7d*E (JD2425200 - 30020);
             since JD2430000 - see Table.
T     Ret    Mean brightness varies with P = 200d.
X     Ret    (k - b)2 = 0.09. P var. Max = 2427425.47 + 0.4920d*E
             [00357]; Max = 2434334.611 + 0.492011d*E (JD2434300 - 600)
             [00080]; since JD2434600 - see Table.
             The shape of the light curve varies. Blazhko effect:
             Pi >= 45d; 0.13P <= M - m <= 0.23P [00080].
R     Sge    P var (70.07d <= P <= 71.24d [09769]. Period variation
             study [00767]. The elements given in the Table are valid
             since JD2434000. The mean brightness varies:
             Min = 2414402 + 1112.d*E [01357].
S     Sge    SB1 (Porb = 675d [01358]). P var. Max = 2409863.32 +
             8.381968d*E (JD2406600 - 18000); since
             JD2418000 - see Table.
U     Sge    VB A (B 9.6m, 92.0", 318deg). Min II 6.71;
             0.014P <= dI <= 0.024P. In the region of the open cluster
             Col 399. Not a member of the cluster. P var [06224, 08608].
             Mean elements are given in the Table representing
             epochs of Min within  +-0.008P. The shape of the light
             curve varies.
V     Sge    VB A (B 13.9m, 9.7", 267deg); SB2 (K1 = 320 km/s,
             K2 = 85 km/s). P var? The depth of eclipses
             varies from 0.6m to 1.3m. The mean brightness outside
             eclipses varies. There are also flares with amplitudes up
             to 3m and small light variations with a time
             scale of minutes, dozens of minutes and a few days.
             spectrum description [03593, 09472].
X     Sge    VB A (B 13.18m, 6", 248deg).
Z     Sge    V1 (NGC 6838, M71). Globular cluster member. P var.
             Max = 2437870 + 175.3d*E (JD2437000 - 38700); since
             JD2438700 - see Table.
RS    Sge    The mean brightnese varies: Max = 2435999 + 1124d*E [08104].
             Two Algol-like light weakenings were also
             observed: JD2444837.22, 2444865.17 [09727].
RW    Sge    P var. according to [01363] Max = 2424289 + 429d*E. Since
             JD2434000 - see Table.
RZ    Sge    Porb ~97m [09771]. Mean cycle is given according to [09785].
             Supermaxima are repeated with the cycle 266d. The period
             of superhumps decreases from 101.3m till 100.8m.
SY    Sge    Min II 10.7. P var. Elements given in the Table are valid
             in the interval JD2425800 - 38300.
TU    Sge    d = 0.035P.
TX    Sge    P var. Max = 2425002 + 155.0d*E (JD2414900 - 25100);
             since JD2425000 - see Table.
UU    Sge    VB A (B 16.5m B, 4", 90deg). The nucleus of the planetary
             nebula Abell 63. Min II 14.41; d = 0.019P.
             The range of the combined light variation is given.
             The actual depth of Min I is about 4.3m. Large reflection
             effect.
UZ    Sge    Min II 11.6:. P var. Min I = 2429961.231 + 2.215750d*E
             (JD2429000 - 41600); since JD2441600 - see Table.
VZ    Sge    VB A (B 12m, 28.2", 206deg).
WY    Sge    Nova Sge 1783 (Max JD2372494:). Min I = 2445137.8993 +
             0.1536342d*E; D = 0.16P. Brightness outside eclipses is
             usually ~18.7m, the depth of the eclipses is ~ 1.5 - 2m.
             At present outbursts by 1.6m are sometimes observed
             similar to the UG type variable outbursts, as well as
             rapid flickering of light [09708].
WZ    Sge    Nova Sge 1913, 1946, 1978. VB A (B 15.76m B, 7", 280deg).
             Really it is not a nova. Three outbursts were registered
             up to day: JD2420094, 32001, 43844 [09710, 09711].
             There are superhumps on the light curve during the
             outburst with 0.057250d >= P >= 0.05714d (A=0.3m V)
             [09710, 09776]. There are light variations between
             the outbursts (A = 0.14m - 0.3m). During some of light
             weakenings Algol-like eclipses are observed (A = 0.2m)
             with the elements: Min I = 2437547.72845 + 0.0566878455d*E
             [09774]; D = 0.04P. d = 0.02P. There are also rapid light
             oscillations (A <= 0.01m). The periods of these
             oscillations before the 1978 outburst were 28.98s and
             27.87s [09774], but after this outburst - 28.95963s [09775].
             According to [09777], in 1976 - 78 these oscillations were
             represented by the elements: Max = 2443311.790250 +
             0.00032254826d*E + 9.8d*10**(-16)*E**2.
XY    Sge    According to [03705] the spectrum is earlier than M0.
AG    Sge    P = 117d?
BR    Sge    d = 0.030P.
CP    Sge    Min II 13.3.
CU    Sge    Min II 11.3.
CW    Sge    Min II 11.7. P var? The shape of the light curve varies.
CZ    Sge    Min II 15.2.
DH    Sge    The shape of the light curve varies (1.1m <= A <= 1.7m).
             P var. Max = 2427612.509 + 0.4695844D*E (JD2427600 -
             38800) [04027]; since JD2438800 - see Table.
             Blazhko effect disappeared after the period change
             (A = 1.1m).
DI    Sge    P var. Max = 2427929 + 203.0d*E (JD2427500 - 30200)
             [02641]; since JD2437100 - see Table.
DK    Sge    Min II 13.0.
DL    Sge    Min II 11.5.
DM    Sge    Min II 11.6.
DP    Sge    P var. Max = 2427985.464 + 0.4883395d*E (JD2427985 - 33000);
             Max = 2432855.191 + 0.4883339d*E (JD2433000 - 40775);
             since JD2440775 - see Table.
DQ    Sge    Min II 14.8.
DS    Sge    Min II 16.0:.
DT    Sge    d = 0.05P:.
EH    Sge    VB A (B 15.6m).
EI    Sge    Min II 14.6.
ER    Sge    P var. Max = 2430515.460 + 0.4184209d*E
             (JD2427000 - 38400);
             Max = 2438443.388 + 0.4184356d*E (JD2438400 - 41800);
             since JD2441800 - see Table.
FF    Sge    d = 0.03P; Min II 13.0.
FG    Sge    VB A (B 14.2m, 8", 100deg). The central star of the
             planetry nebula PK 60deg (diameter 36", the age about 6000
             years). The brightness of the star steadily increased from
             13.6 pg in 1894 to the maximum in 1967, and then is
             steadily decreasing. In 1982 it was 11.0 B. In 1967 the
             strong absorption lines of rare earth elements appeared
             in the spectrum. The spectral class steadily becomes
             later. The signes of new planetary nebula ejection were
             observed. In 1962 the star entered the instability
             strip in the Mv, B-V diagram and began to pulsate
             with a small amplitude and increasing period: Min(V) =
             2442629 + 59.83d*E + 1.126d*E**2 (JD2442600 - 44530).
             In twenty years the period increased from 50d to 134d,
             the amplitude of pulsations changed from 0.2mV to 0.5mV;
             now it decreased again to 0.2mV, and the period is only
             90d [09780].
FH    Sge    Min II 13.5.
FL    Sge    There is a close companion 14m. In the minimum probably
             fainter than 15.9m.
FO    Sge    P var. Max = 2427578.0 + 67.8d*E (JD2427570 - 28120);
             Max = 2428134.4 + 72.7d*E (JD2428120 - 30150);
             since JD2430150 - see Table.
FP    Sge    Min II 14.9. P = 0.32100275d?
FT    Sge    P.K.55-1 deg 2. Not a planetary nebula.
FU    Sge    Min II 15.8.
FX    Sge    In the region of the globular cluster M71 (NGC 6838).
GI    Sge    Red.
GN    Sge    Min II 10.6.
GP    Sge    Red.
GY    Sge    P var. Max = 2431264.49 + 51.497d*E (JD2429490 - 34900)
             [07199]; Max = 2433787.42 + 51.5991d*E (JD2433600 - 37280),
             Max = 437911.04 + 51.2524d*E (JD2437280 - 40510) [06172];
             since JD2444450 - see Table.
HH    Sge    The cycles 23 - 26d and 300d are observed.
HM    Sge    VB A (B 14.20m, 10", 182deg). The brightness increased
             from 17.2m up to 11.3m pg in the interval JD2442280 -
             42650. Then the light variations in the infrared region
             appeared with P = 550d [09721, 09783] and A(K) = 1.5m.
             Radio and X-ray source.
IR    Sge    SF star in a close pair.
LN    Sge    SF star in a close pair.
MV    Sge    Possible member of the globular cluster Palomar 10.
MZ    Sge    Possible member of the globular cluster Palomar 10.
PT    Sge    P component of a close pair.
V0339 Sge    Extremely metal-weak.
del   Sge    VB A (B, A = 0.04", P = 7 yr); SB2 (Porb = 3725d [09789]).
             The last superior conjunction of the B-star and its
             atmospheric eclipse was in March - April 1980 [09726].
R     Sgr    P var. Max = 2405776 + 271.0d*E (JD2399500 - 2407500);
             Max = 2407115 + 264.2d*E (JD2407100 - 9500);
             Max = 2418125 + 269.65d*E (JD2409500 - 19500);
             Max = 2433137 + 267.90d*E (JD2419500 - 36000);
             since JD2436000 - see Table.
S     Sgr    P var. Max = 2401029 + 230.6d*E (JD2401000 - 10000);
             Max = 2411638 + 229.2d*E (JD2410000 - 19500);
             Max = 2422222 + 232.81d*E (JD2419500 - 27000);
             since JD2427000 - see Table.
T     Sgr    Companion F3IV (ro < 0.8"). P var.
             Max = 2409013 + 385.1d*E (JD2401500 - 10500);
             Max = 2414582 + 399.0d*E (JD2413000 - 17500);
             Max = 2424363 + 387.9d*E (JD2417500 - 25500);
             since JD2425500 - see Table.
             S 5/6-e. There are Te lines and a very strong
             Li lambda 6708 line in the spectrum.
U     Sgr    The member of the open  cluster M25 (IC 4725).
             P var. Max = 2416628.046 + 6.744925d*E (JD2404480 - 30115)
             [00765]; since JD2430115 - see Table. [A/H] = 0.1.
W     Sgr    VB A (A 9.2m, 0.116", 153.3deg, 1976.477; B 13.5m, 33.4",
             233deg; C 13.5m, 47.9", 101deg). P var.
             Max = 2403198.39 + 7.594695d*E (JD2403100 - 34500); since
             JD2434500 - see Table.
X     Sgr    P var. Max = 2410006.22 + 7.01206d*E (JD2403000 - 17000);
             Max = 2424248.11 + 7.01245d*E (JD2417000 - 34500); since
             JD2434500 - see Table.
Y     Sgr    In the region of the open cluster M25 (IC 4725).
RR    Sgr    P var. Max = 2410008 + 336.0d*E (JD2410000 - 17100)
             [09794]; Max = 2422755 + 332.73d*E (JD2422700 - 32100)
             [00960]; since JD2432100 - see Table. OH, H2O emission.
RS    Sgr    VB A (B 9.65m V, 39.0", 86deg). Min II 6.28.
RT    Sgr    P var. Max = 2412759 + 303.1d*E (JD2412700 - 8300)
             [00960]; Max = 2425588 + 308.8d*E (JD2422800 - 26700);
             Max = 2428034 + 303.8d*E (JD2426700 - 33500);
             since JD2433500 - see Table.
RU    Sgr    P var. Max = 2413062 + 242.3d*E (JD2410150 - 16700)
             [00960]; Max = 2423670 + 242.3d*E (JD2422500 - 24500);
             Max = 2428200 + 237.6d*E (JD2424500 - 28800); since
             JD2428800 - see Table.
RV    Sgr    P var. Max = 2411206 + 319.3d*E (JD2410200 - 17000)
             [00960]; Max = 2429032 + 321.3d*E (JD2422600 -
             29500); since JD2429500 - see Table.
RW    Sgr    P var. Max = 2413798 + 189.0d*E (JD2413700 - 23000);
             Max = 2431998 + 190.87d*E (JD2423000 - 33500);
             since JD2433500 - see Table.
RX    Sgr    P var. Max = 2417730 + 330.3d*E (JD2413000 - 18500);
             Max = 2420122 + 346d*E (JD2418500 - 20150);
             Max = 2420122 + 323d*E (JD2420100 - 22200);
             Max = 2424120 + 345d*E (JD2422200 - 24200);
             Max = 2428785 + 332.2d*E (JD2424000 - 31500);
             since JD2431500 - see Table.
RY    Sgr    VB A (B 15.69m, 12"). There are pulsational light
             variations (0.1m < A < 1.5m) with the elements:
             Max = 2433670 + 38.6056d*E - 78d*10**(-5)*E**2.
             light curve [09798, 09799]; spectrum description [06261].
ST    Sgr    S 6/3-e.
SU    Sgr    VB A (B 13.5m, 1.0", 240deg, 1932.45).
             earlier P = 88d was observed [00017].
SV    Sgr    In the nebula M8 (NGC 6523).
SW    Sgr    P var. Max = 2416338 + 290.3d*E (JD2414000 - 16500);
             Max = 2428507 + 288.5d*E (JD2422500 - 29000);
             Max = 2429088 + 293.5d*E (JD2429000 - 33000);
             since JD2433000 - see Table.
SX    Sgr    Min II 9.62; d = 0.05P. P var. Min I = 2429114.249 +
             4.15395762d*E (JD2410000 - 29150) [00007];
             since JD2429000 - see Table.
SY    Sgr    In the region of the nebula S188.
SZ    Sgr    VB A (B 12.5m V, 2.0", 212deg.)
VV    Sgr    In the region of the open cluster NGC 6494. OH, H2O
             emission.
VX    Sgr    P var; 1m <= A <= 6m. SIO, H2O, OH maser.
             Light curve (1935-1969) [06615].
VY    Sgr    [A/H] = 0.5.
WX    Sgr    VB A (B 12.5m, 0.4", 88deg). P var. Min = 2419317.259 +
             2.129095d*E (JD2419300 - 24700) [00457]; Min =
             2424729.418 + 2.129113d*E (JD2424700 - 39700)
             [00279]; since JD2440000 - see Table.
WY    Sgr    Min II 10.3.
WZ    Sgr    The member of the open cluster C 1814-190. [A/H] = 0.4.
XX    Sgr    P var. Max = 2419189.730 + 6.424264d*E (JD2419100 - 30100)
             [00637]; since JD2435000 - see Table.
XZ    Sgr    Min II 8.95; d = 0.022P. P var. Min I = 2420311.519 +
             3.275537d*E (JD2420300 - 28000) [01604]; Min I =
             2436440.137 + 3.27549d*E (JD2428000 - 37500)
             [02516]; Min I = 2441150.348 + 3.2755357d*E
             (JD2437500 - 41500) [07084]; since JD2441500 - see Table.
YY    Sgr    Min II 10.64; Min II = 2433075.8296 + 2.628463d*E
             [02302]. Apsidal motion period is about 300 years.
AL    Sgr    P var. Max = 2425792 + 79.07d*E (JD2421000 - 26000);
             since JD2426000 - see Table.
AN    Sgr    P var. Max = 2425720 + 339.62d*E (JD2415000 - 26000);
             Max = 2428360 + 330.0d*E (JD2426000 - 28500);
             since JD2428500 - see Table.
AP    Sgr    SB? [09004].
AR    Sgr    There is a square term in the elements:
             -[0.0031d (E-30)**2 + 8.8d].
AS    Sgr    Planetary nebula HB6 = 7 + 1deg 1.
AU    Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6514 (M20).
AV    Sgr    In the region of the open cluster NGC 6546. Not a member
             of the cluster. [A/H] = 0.4. P var.
             Max = 2429083.30 + 15.4093d*E (JD2421400 - 39100); since
             JD2439100 - see Table.
AW    Sgr    VB A (B 16m, 15", 97deg).
             In the region of the open cluster NGC 6546.
AY    Sgr    [A/H] = 0.2.
BB    Sgr    VB A (B = V4088 Sgr, 7.49m - 7.87m, 93.5", 102deg).
             In the region of the open cluster Cr394.
BE    Sgr    A var (0.6m <= A <= 1.1m).
BM    Sgr    P var.
BN    Sgr    Min II 9.37; d = 0.04P:.
             Soft X-ray source. P var [01600].
BQ    Sgr    d = 0.017P. P var. Min = 2412592.7905 + 8.01964d*E
             (JD2412590 - 22220) [01696]; since JD2422220 - see Table.
CC    Sgr    In the region of the globular cluster NGC 6723.
CD    Sgr    In the region of the globular cluster NGC 6723. P var.
             Max = 2416247 + 266.62d*E
             (JD2411000 - 23000); since JD2423000 - see Table.
CE    Sgr    In the region of the globular cluster NGC 6723.
             SF component of a close double.
CF    Sgr    In the region of the globular cluster NGC 6723.
             P var. Max = 2415632.81 + 0.570026d*E (JD2411000 -
             23800) [01616]; since JD2423900 - see Table.
CG    Sgr    In the region of the globular cluster NGC 6723.
DH    Sgr    In the region of the globular cluster NGC 6809 (M55).
DI    Sgr    In the region of the globular cluster NGC 6809 (M55).
DK    Sgr    In the region of the globular cluster NGC 6809 (M55).
DM    Sgr    In the region of the globular cluster NGC 6809 (M55).
DO    Sgr    In the region of the globular cluster NGC 6809 (M55).
DP    Sgr    In the region of the globular cluster NGC 6809 (M55).
DR    Sgr    In the region of the globular cluster NGC 6809 (M55).
DS    Sgr    In the region of the globular cluster NGC 6809 (M55).
DV    Sgr    d = 0.044P.
EG    Sgr    d = 0.010P.
FV    Sgr    P var. Max = 2424010 + 269.5d*E (JD2424000 - 27500)
             [00251]; since JD2427500 - see Table.
GG    Sgr    P var. Max = 2413840 + 286.5d*E (JD2413800 - 24000);
             since JD2424000 - see Table.
GK    Sgr    According to [05869] - eclipsing.
GU    Sgr    There are also light variations with <P> = 37.5d,
             0.4m <= A(V) <= 1.5m [06273].
HH    Sgr    VB (ro = 0.1').
IR    Sgr    VB B (A 13.6m; B 10", 220deg).
KO    Sgr    Similar to UG. It is possible that the observations in Min
             brightness refer to a companion.
LZ    Sgr    VB A (B 16m, 7", 30deg).
MV    Sgr    Very hot hydrogen deficient extreme helium carbon star.
MW    Sgr    P var. Max = 2418940 + 202.3d*E (JD2418900 - 23900);
             Max = 2428753 + 206.5d*E (JD2423900 - 28950);
             since JD2428950 - see Table.
NP    Sgr    The cycles 100 - 300d are possible.
OW    Sgr    In the region of the open cluster NGC 6716.
V0348 Sgr    VB A (B 15m pg, 16", 73deg). Very hot hydrogen deficient
             helium carbon star.
             By the character of light variation and the spectrum the
             star is unique. The light curve resembling those of RCB
             type stars is superimposed by conspicuons irregular and
             semiregular variations with the mean cycle about 200d
             [02449, 09824]. The star is surrounded by a nebula the
             radius of which equals 1". A fainter nebulous envelope is
             observed up to 7" from the star. Large infrared
             excess. Spectrum description [02451, 09825]. Probably
             the star is intermediate between the RCB variables
             And planetary nebula Wolf-Rayet central stars.
V0350 Sgr    SB [09004].
V0354 Sgr    d = 0.02P.
V0356 Sgr    Min II 7.24; DII = 0.20P:; d = 0.05P;
             0.490P (1928) <= Min II - Min I <= 0.505P (1951).
             Apsidal motion is possible.
V0366 Sgr    P var. Max = 2425479.448 + 0.4779616d*E (JD2423990 - 28780)
             [00705]; since JD2435600 - see Table. [Ca/H] = -0.73.
V0367 Sgr    [Ca/H] = -1.21.
V0377 Sgr    The epoch of light min is given in the Table.
             P var. Min = 2426071.24 + 16.17076d*E (JD2425300 - 26600)
             [00048]; Min = 2427350.25 + 16.19326d*E (JD2426600 - 28700)
             [01400]; Min = 2436358.98 + 16.1575d*E
             (JD2436200 - 37300); Min = 2437863.09 + 16.1925d*E
             (JD2437660 - 39100); Min = 2440114.81 + 16.2407d*E
             (JD2440200 - 560); since JD2440950 - see Table.
V0397 Sgr    There is a square term in the elements:
             -0.009d*10**(-6)*E**2
V0401 Sgr    Min II 14.1.
V0403 Sgr    There is a nonlinear term in the elements:
             -0.013d*10**(-6)*E**2.
V0410 Sgr    VB A (B 13.6m, 270deg).
V0426 Sgr    Min II 13.3.
V0427 Sgr    There is a nonlinear term in the elements:
             -131d*10**(-10)*E**2. The shape of the light curve varies:
             0.17P <= M - m <= 0.22P.
V0431 Sgr    Min II 14.9.
V0437 Sgr    Min II 14.0.
V0440 Sgr    Delta(S) = 9. P var. P = 0.4774659d (JD2416000 - 23000)
             [00752]; P < 0.4774659d (JD2422000 - 26000) [00235];
             Max = 2426581.203 + 0.477474d*E (JD2426000 - 29460) [01000];
             since JD2437100 - see Table.
V0453 Sgr    There is a nonlinear term in the elements:
             +0.003d*10**(-6)*E**2.
V0457 Sgr    There is a nonlinear term in the elements:
             -0.005d*10**(-6)*E**2.
V0466 Sgr    There is a nonlinear term in the elements:
             +0.03d*10**(-6)*E**2.
V0496 Sgr    Min II 14.3.
V0497 Sgr    Min II 16.0.
V0505 Sgr    Min II 6.63. P var. Min I = 2433515.3295 + 1.18287141d*E
             (JD2425500 - 35800) [01642]; Min I = 2437494.4964 +
             1.1828622d*E (JD2435800 - 37500); Min I =
             2440055.3991 + 1.1828650d*E (JD2437500 - 40100);
             Min I = 2442656.5283 + 1.18286917d*E (JD2440100 -
             42670); since JD2442670 - see Table. The shape of the
             light curve varies. Deviations from the mean light curve
             vary with P = 310d. The difference of Min I and Min II
             depths varies by 0.05m [09830].
V0511 Sgr    P var. Max = 2423950 + 158.8d*E (JD2411300 - 23950);
             since JD2423950 - see Table.
V0515 Sgr    There is a nonlinear term in the elements: +0.015d*E**2.
V0519 Sgr    There is a nonlinear term in the elements: +0.0046d*E**2.
V0520 Sgr    There is a nonlinear term in the elements: +0.051d*E**2.
V0523 Sgr    Min II 9.88. Apsidal motion is observed. In the Table the
             epoch of Min I is given corresponding to the moment of
             line of apsides coinciding with the line of sight, when
             Min II - Min I = 0.50P. The mean period according to
             [02453] is given; with this period O - C deviations do not
             exceed  +-0.06P for both minima. The period of apsidal
             motion is 248 years [02453]. Min II - Min I = 0.39P in 1953.
V0524 Sgr    Min II 11.2.
V0525 Sgr    Min II 8.51.
V0526 Sgr    VB A (B 12.40m, 8.6", 7.3deg). Min II 10.20, DII = 0.17P;
             dI = 0.006P, dII = 0.013P.
             There are periodic terms in the elements:
             +0.1369d*sin(0.01295deg*E) - 0.0115d*sin(0.0259deg*E) +
             0.0011d*sin(0.0388deg*E). Min II = 2422055.0453 +
             1.919411d*E - 0.1369d*sin(0.01295deg*E) -
             0.0115d*sin(0.0259deg*E) - 0.0011d*sin(0.0388deg*E).
             The period of apsidal motion is 146 years. e = 0.224.
V0527 Sgr    P var. Max = 2426904.95 + 1.258956d*E (JD2425790 - 7650)
             [01648]; since JD2438200 - see Table.
V0551 Sgr    VB B (A 16.5m; B 12", 135deg).
V0552 Sgr    P var. The elements given in the Table are
             valid since JD2418400.
V0554 Sgr    Min II 14.5.
V0557 Sgr    P var. Max = 2415110.5 + 16.233d*E (JD2415100 - 22000);
             Max = 2426100.0 + 16.260d*E (JD2423900 - 27700) [00251];
             Max = 2428097.70 + 16.171d*E (JD2427700 - 28800) [00296];
             since JD2428800 - see Table.
V0558 Sgr    Min II 14.3.
V0564 Sgr    P var. Max = 2424056 + 27.8d*E (JD2423780 - 26000)
             [00251]; Max = 2428403.3 + 27.99d*E (JD2427870 - 29160)
             [00296]; Max = 2429158.2 + 27.2d (JD2429150 - 515);
             since JD2429515 - see Table.
V0567 Sgr    The central star of the planetary nebula P.K.355 -6deg 1
             (M3-21).
V0573 Sgr    Min II 12.7.
V0574 Sgr    Min II 14.7.
V0578 Sgr    According to [02448], Max = 2428710 + 253d*E.
V0593 Sgr    P var. Max = 2414150 + 230d*E (JD2414100 - 22900);
             since JD2423900 - see Table.
V0598 Sgr    d = 0.05P.
V0611 Sgr    P var. Max = 2414150 + 123d*E (JD2414150 - 19000);
             since JD2420250 - see Table.
             The period must probably be doubled because the star
             resembles RV Tau (Min II 16.2).
V0612 Sgr    P var. Max = 2413750 + 107.9d*E (JD2413700 - 17900);
             since JD2418800 - see Table.
V0615 Sgr    P.K.356 -7deg 1 = He 2-349.
V0626 Sgr    P var? Max = 2427715.4 + 26.745d*E (JD2425380 - 28800)
             [00046]; since JD2434500 - see Table.
V0631 Sgr    Min II 14.2.
V0632 Sgr    P var. Max = 2413350 + 263d*E (JD2413300 - 19000);
             since JD2420200 - see Table.
V0633 Sgr    P var. Max = 2415110 + 224d:*E (JD2415000 - 18800);
             since JD2420000 - see Table.
V0638 Sgr    P var? Max = 2412670 + 73.1d*E (JD2412600 - 14540);
             since JD2414800 - see Table.
V0646 Sgr    P var. Max = 2413350 + 95d*E (JD2413300 - 15900);
             since JD2423900 - see Table.
V0660 Sgr    P var. Max = 2426460 + 235.6d*E (JD2426400 - 35700)
             [00251]; since JD2435600 - see Table.
V0663 Sgr    P var. Max = 2426160 + 305d*E [00251];
             since JD2435600 - see Table.
V0671 Sgr    P = 292.5d?
V0672 Sgr    P var? Max = 2424680 + 228d*E [00251]; since
             JD2435600 - see Table.
V0674 Sgr    P var. Max = 2425830 + 249d*E [00251]; since
             JD2435600 - see Table.
V0675 Sgr    (k - b)2 = -0.01; Delta(S) = 11.
V0676 Sgr    P var. Max = 2414140 + 181d*E (JD2414100 - 22600)
             [00251]; since JD2423900 - see Table.
V0679 Sgr    P var. Max = 2415900 + 225d*E (JD2415900 - 22200)
             [00251]; Max = 2425440 + 223.1d*E (JD2425000 - 29000);
             since JD2429000 - see Table.
V0683 Sgr    Min II 12.5.
V0686 Sgr    P var? Max = 2425390 + 225.3d*E [00251]; since
             JD2435600 - see Table.
V0687 Sgr    Min II 12.2.
V0691 Sgr    P var? Max = 2426095.550 + 0.46911d*E [00251];
             since JD2435630 - see Table.
V0703 Sgr    Var 4. According to [02951] the range of light variation,
             the type of variability and the elements of light
             variation are erroneously assigned in [01640] to the star
             Var 3.
V0705 Sgr    Min II 12.9.
V0710 Sgr    P var. Min = 2426101.550 + 2.3817d*E [00251]; Min =
             2431286.425 + 2.381633d*E (JD2428390 - 35700) [03513].
V0713 Sgr    P var? Max = 2424680 + 253.4d*E [00251]; since
             JD2435600 - see Table.
V0716 Sgr    P var? Max = 2424670 + 277d*E [00251]; since
             JD2435600 - see Table.
V0718 Sgr    P var? Max = 2425850 + 153.2d*E [00251]; since
             JD2435600 - see Table.
V0721 Sgr    P = 71:d?
V0725 Sgr    Unique star.
             The mean brightness increased from 13.0m to 12.4m
             since 1889 to 1915, and fell to 12.8m in 1926. From
             1895 to 1926 real shortperiodic oscillations with the
             amplitude about 0.4m. In 1928 the amplitude suddenly
             increased by almost 2m, but the magnitude in maximum
             remained unchanged. From 1928 to 1935 the light
             variations became periodic, the period increasing every
             year by 1d in accordance with the formula:
             Min = 2426087 + 15.933d*E + 0.0233d*E**2.
             In 1935 P = 21d. Since 1936 only small oscillations of
             brightness with a gradual increase of the mean magnitude
             from 14.3m to 13.9m B (1969). Photoelectric observations
             in 1968 - 69 reveal the light variations 12.33m - 12.72m V
             with possible periods 15.4d in 1968 and 45.3d in 1969. In
             1973 12.28m - 12.58m V, <B-V> = +1.37, P = 50d [07101].
V0727 Sgr    VB A (B = V728 Sgr, 14.7m - 15.9m, 25", 108deg).
V0728 Sgr    VB B (A = V727 Sgr, B 25", 108deg).
V0734 Sgr    Min II 13.1.
V0735 Sgr    VB A (B 15.5m, 6", 315deg). According to B-V, U-B values
             and spectrum the star is not a UG type variable [09840].
V0738 Sgr    In the region of the globular cluster NGC 6558.
             According to [05403], RV? P = 86.78d?
V0743 Sgr    Min II 14.2.
V0745 Sgr    P var. Max = 2416560 + 385.1d*E (JD2411000 - 19260);
             since JD2419260 - see Table.
V0748 Sgr    Min II 14.7; d = 0.04P.
V0750 Sgr    d = 0.02P:.
V0752 Sgr    Min II 12.7.
V0755 Sgr    d = 0.01P.
V0757 Sgr    Min II 13.8; d = 0.06P.
V0760 Sgr    Min II 13.4. P var. Min = 2414059.5 + 45.10d*E
             (JD2412800 - 19000); since JD2419000 - see Table.
V0761 Sgr    Min II 12.8; d = 0.05P.
V0762 Sgr    P var. Max = 2414100 + 461d*E (JD2411000 - 22860);
             since JD2422860 - see Table.
V0763 Sgr    P var. The observations are satisfied by the given
             elements since JD2415000.
V0766 Sgr    d = 0.05P.
V0768 Sgr    Min II 13.0.
V0770 Sgr    Min II 13.1.
V0773 Sgr    [A/H] = 0.1.
V0777 Sgr    d = 0.055P.
V0778 Sgr    Min II 12.1.
V0779 Sgr    Min II 12.0.
V0780 Sgr    Min II 12.9; d = 0.08P.
V0782 Sgr    d = 0.045P.
V0784 Sgr    Min II 12.8.
V0786 Sgr    d = 0.025P.
V0789 Sgr    In the region of the open cluster Tr 31.
             P = 5.10470d (Min II 12.7)? [00478].
V0791 Sgr    d = 0.03P:.
V0792 Sgr    Min II 12.2. In the region of the open cluster
             and the diffuse nebula NGC 6514 (M 20).
V0793 Sgr    P var. Max = 2412610 + 195d*E (JD2412600 - 19400);
             since JD2423400 - see Table.
V0794 Sgr    P var. Min I = 2413723 + 173.48d*E (JD2413700 -
             23750); since JD2423750 - see Table.
V0801 Sgr    Min II 14.9.
V0802 Sgr    [A/H] = -0.4.
V0803 Sgr    P = 3.771748d?
V0818 Sgr    The shape of the light curve varies.
V0819 Sgr    P var?
V0824 Sgr    Min II 15.2.
V0828 Sgr    There is a close companion.
V0838 Sgr    P var?
V0839 Sgr    P var? Max = 2426170.126 + 1.835347d*E (JD2425700 - 26600)
             [01598]; since JD2441500 - see Table.
V0841 Sgr    The shape of the light curve varies.
V0844 Sgr    P var?
V0845 Sgr    Min II 14.6.
V0859 Sgr    The shape of the light curve varies.
V0879 Sgr    There is a close companion.
V0882 Sgr    Min II 14.6.
V0884 Sgr    0.20P <= M - m <= 0.40P. Blazhko effect.
V0889 Sgr    0.14P <= M - m <= 0.24P. Blazhko effect.
V0902 Sgr    Min II 14.8.
V0903 Sgr    Min II 13.0.
V0919 Sgr    Spectrum description [09845].
V0935 Sgr    P var. Max = 2420040 + 232.0d*E (JD2419500 - 28650);
             since JD2428600 - see Table.
V0938 Sgr    P = 138.27d?
V0960 Sgr    nP = 1734d.
V0966 Sgr    Min II 14.0.
V0977 Sgr    d = 0.03P.
V0981 Sgr    Min II 14.8.
V0985 Sgr    Min II 14.3.
V0986 Sgr    d = 0.015P.
V0993 Sgr    dI = 0.05P:; Min II 13.7, DII = 0.09P, dII = 0.00P.
V0994 Sgr    Min II 12.8:.
V0998 Sgr    The depth of Min II 0.04m:.
V1000 Sgr    Min II 13.9.
V1002 Sgr    Min II 13.7.
V1004 Sgr    [A/H] = -0.2.
V1005 Sgr    Min II 13.9.
V1013 Sgr    Min II 15.0.
V1017 Sgr    VB B (A 10.6m V; B 15", 270deg).
             For a long time the star was considered to be a recurrent
             nova. Three considerable flares were observed: in 1901
             (10.8m), 1919 (6.2m), and 1973 (10.5m). Composite spectrum
             with a trace of a hot component [03872].
V1023 Sgr    In the region of the open cluster Cr 394. Min II 13.0:.
V1026 Sgr    Min II 13.4.
V1028 Sgr    Min II 14.4.
V1032 Sgr    Min II 15.0.
V1033 Sgr    The shape of the light curve varies. Blazhko effect?
V1034 Sgr    d = 0.025P:.
V1049 Sgr    Min II 13.6; Min II - Min I = 0.326P; DII = 0.025P.
V1050 Sgr    Min II 14.1.
V1056 Sgr    Min II 14.1.
V1063 Sgr    The shape of the light curve strongly varies. Blazhko
             effect?
V1068 Sgr    Min II 15.4.
V1069 Sgr    The shape of the light curve strongly varies. Blazhko
             effect?
V1071 Sgr    P = 1.3560996d?
V1072 Sgr    The shape of the light curve strongly varies. Blazhko
             effect?
V1080 Sgr    P var. The shape of the light curve varies.
V1081 Sgr    P var?
V1089 Sgr    Cycle <= 30d.
V1100 Sgr    d = 0.02P:.
V1108 Sgr    Min II 11.9; Min II - Min I = 0.516P.
V1109 Sgr    Min II 14.5.
V1127 Sgr    There is a nonlinear term in the elements:
             +78.10d**(-10)*E**2.
V1136 Sgr    d = 0.020P.
V1148 Sgr    In the region of the globular cluster NGC 6553.
V1153 Sgr    P var? Max = 2428391.266 + 1.332624d*E (JD2427680 -
             30910); since JD2435630 - see Table.
V1177 Sgr    Min II 11.4.
V1178 Sgr    d = 0.03P:.
V1180 Sgr    [A/H] = -0.4.
V1181 Sgr    [A/H] = 0.6. P var. Max = 2428452.25 + 21.341d*E
             (JD2427400 - 31000) [01638]; since JD2433000 - see Table.
V1185 Sgr    [A/H] = -0.5. P var. Max = 2428778.86 + 13.9123d*E
             (JD2427500 - 32750) [01638]; Max = 2437485.4 +
             13.901345d*E (JD2437100 - 43760) [08519];
             since JD2444000 - see Table.
V1187 Sgr    [A/H] = -0.8.
V1188 Sgr    [CA/H] = -0.37.
V1189 Sgr    [A/H] = -1.1.
V1190 Sgr    P = 3.000078d?
V1191 Sgr    Min II 14.4.
V1205 Sgr    The alternative period is possible: 0.659820d [01638].
V1209 Sgr    A var.
V1211 Sgr    Delta(S) = 3:.
V1214 Sgr    There is a nonlinear term in the elements:
             -0.25d*10**(-7)*E**2.
V1216 Sgr    mu = 0.720", P = 106.7deg.
V1223 Sgr    As a rule has a persistent high state; five drops by two
             to more than three magnitudes have been registered and a
             twelve year interval of irregular variations at
             intermediate magnitudes. According to [09850] there are
             slow variations in brightness by 0.15m on a time scale
             of ~1 day. They are superimposed by variations with the
             orbital period P orb (Max = 2444749.9866 + 0.140239d*E)
             and with amplitude up to 0.15m. These variations in their
             turn are superimposed by the others: with P = 794.38s
             and the amplitude from 0.03m up to 0.15m
             (Max = 2444750.00404 + 0.009194215d*E and (sometimes) with
             P = 849.8s and a twice smaller amplitude
             (Max = 2444750.00350 + 0.00983588d*E). Besides there are
             rapid brightness variations on time scales 10 - 100s by
             0.10m - 0.20m, and high frequency flickering by 0.05m.
             According to [09851], the period of X-ray pulses associated
             with the rotation of the compact object is 12.5 minutes.
V1276 Sgr    Min II 14.3.
V1280 Sgr    Brightness of Max varies by 2m with the period 5230d.
V1281 Sgr    The light variation is not strictly periodic.
V1282 Sgr    P var. Min = 2427651.297 + 1.754574d*E (JD2427650 -
             30560) [00705]; since JD2435600 - see Table.
V1284 Sgr    Min II 13.5. EB?
V1287 Sgr    Var 3. According to [02951] the range of light variation of
             Var 4 (V703 Sgr), the type of variability and the elements
             of light variation of Var 4 (V703) are erroneously
             assigned in [01640] to the star Var 3.
             According to [02951] the range of light variation, the type
             of variability and the elements of light variation are
             erroneously assigned in [01640] to the star Var 4.
             Min II 14.8.
V1290 Sgr    [A/H] = -1.2.
V1303 Sgr    [A/H] = -0.8. P var? Max = 2438241.176 + 18.46812d*E
             (JD2427700 - 38250) [00001]; since JD2444000 - see Table.
V1304 Sgr    [A/H] = 0.3. P var. Max = 2428758.10 + 12.9287d*E
             (JD2427590 - 28820) [01640]; since JD2435600 - see Table.
V1309 Sgr    Not far from V4032 Sgr.
V1311 Sgr    V 14 in the globular cluster NGC 6656 (M22).
             Not a member of the cluster.
V1312 Sgr    P var? Max = 2428815.600 + 0.6011427d*E (JD2427590 - 28820)
             [01640]; since JD2435630 - see Table.
V1314 Sgr    P var? Max = 2428346.536 + 0.657489d*E (JD2427600 -
             28820) [01640]; since JD2435630 - see Table.
V1317 Sgr    P var?
V1327 Sgr    SR?, L? [08424].
V1328 Sgr    P = 0.39937d?
V1329 Sgr    VB B (A 17.2m; B 1.4", 120deg). P var. Max = 2432388.777 +
             0.48306d*E (JD2431670 - 32740) [03524];
             since JD2443300 - see Table.
V1331 Sgr    Min II 16.5.
V1352 Sgr    P var. Max = 2431998.851 + 0.49505d*E (JD2431670 -
             33150) [01680]; Max = 2443341.844 + 0.49493d*E
             (JD2443300 - 350); Max = 2444087.558 + 0.49516d*E
             (JD2444050 - 110); in the interval JD2444400 - 410 - see
             Table.
V1356 Sgr    Min II 18.0:.
V1357 Sgr    Min II 19.0.
V1359 Sgr    P var?
V1369 Sgr    P var. Max = 2432736.821 + 0.52956d*E (JD2431670 - 33150)
             [03524]; since JD2440700 - see Table.
V1374 Sgr    Delta(S) = 1.
V1378 Sgr    Delta(S) = -3:.
V1387 Sgr    Delta(S) = 3.
V1389 Sgr    The epoch of Min brightness is given.
V1390 Sgr    Min II 17.6.
V1392 Sgr    P var. Max = 2432739.791 + 0.55032d*E (JD2431670 - 33150)
             [03524]; since JD2440700 - see Table.
V1393 Sgr    Delta(S) = 3.
V1394 Sgr    Min II 18.0.
V1401 Sgr    The epoch of Min brightness is given.
V1405 Sgr    P var. Max = 2432031.778 + 0.46511d*E (JD2431670 - 33150)
             [06094]; since JD2443300 - see Table.
V1408 Sgr    A var (0.5m <= A <= 1.4m).
V1409 Sgr    P var. Max = 2432739.822 + 0.65159d*E (JD2431670 - 33150)
             [03524]; since JD2443300 - see Table.
V1412 Sgr    The epoch of Min brightness is given.
V1415 Sgr    P var?
V1416 Sgr    Delta(S) = 3. P var? Max = 2432002.875 + 0.42767d*E
             (JD2431670 - 33150) [06094]; since JD2440700 - see Table.
V1418 Sgr    P var. Max = 2432740.818 + 0.45423d*E (JD2431670 - 33150)
             [03524]; since JD2440700 - see Table.
V1419 Sgr    P var. Max = 2432061.669 + 0.57144d*E (JD2431670 - 33150)
             [01680]; since JD2440700 - see Table.
V1425 Sgr    Min II 18.8.
V1426 Sgr    Delta(S) = 1.5.
V1429 Sgr    The epoch of Min brightness is given.
V1435 Sgr    Min II 18.0; Min II - Min I = 0.53P.
V1437 Sgr    V8 (NGC 6522); not a member of the globular cluster.
V1438 Sgr    V9 (NGC 6522); not a member of the globular cluster.
V1439 Sgr    P = 0.53711d? [06094].
V1443 Sgr    Min II 18.6.
V1446 Sgr    Min II 18.0.
V1447 Sgr    Min II 18.2.
V1454 Sgr    Min II 15.4.
V1457 Sgr    Min II 19.0.
V1459 Sgr    The depth of Min II is 0.04m.
V1460 Sgr    P var. Max = 2432067 + 162.0d*E (JD2431670 - 33150)
             [01680]; since JD2440340 - see Table.
V1464 Sgr    Delta(S) = 1.
V1465 Sgr    P var. Max = 2431702.660 + 0.45757d*E (JD2431700 - 940);
             Max = 2432706.945 + 0.45757d*E (JD2431940 - 32740) [03524];
             since JD2440740 - see Table.
V1466 Sgr    The epoch of Min brightness is given.
V1473 Sgr    According to [08424] P = 340d.
V1487 Sgr    Min II 18.8.
V1491 Sgr    Min II 18.5.
V1498 Sgr    SP component of a close pair. P var.
             Max = 2432739.728 + 0.47467d*E (JD2431670 - 33150) [06094];
             since JD2443300 - see Table.
V1508 Sgr    VB.
V1509 Sgr    Min II 18.1:.
V1510 Sgr    According to [06094], P = 0.48546d.
V1516 Sgr    P var? Max = 2432740.753 + 0.49709d*E (JD2431670 -
             33150) [03524]; since JD2440700 - see Table.
V1517 Sgr    P < 2.0d.
V1523 Sgr    P var? Max = 2432417.702 + 0.36202d*E (JD2431670 - 33150)
             [03524]; since JD2443300 - see Table.
V1526 Sgr    Min II 18.3.
V1537 Sgr    Min II 17.4; Min II - Min I = 0.54P.
V1540 Sgr    According to [08424], P = 465d.
V1546 Sgr    The epoch of Min brightness is given.
V1550 Sgr    P = 0.37432d? [06094].
V1554 Sgr    Min II 17.5.
V1557 Sgr    Delta(S) = 8.
V1558 Sgr    Delta(S) = 1.
V1559 Sgr    The depth of MinII is 0.04m.
V1561 Sgr    Min II 17.7.
V1567 Sgr    Min II 18.0.
V1569 Sgr    Min II 18.6.
V1576 Sgr    [Ca/H] = -1.23.
V1577 Sgr    P var. Max = 2426200 + 290d*E (JD2426000 - 30560)
             [02449]; since JD2430560 - see Table.
V1580 Sgr    P var (310d <= P <= 365d).
V1589 Sgr    [Ca/H] = -0.91.
V1602 Sgr    d = 0.03P.
V1610 Sgr    P < 0.5d.
V1639 Sgr    The shape of the light curve varies.
V1640 Sgr    (k -b)2 = 0.24. P var?
V1642 Sgr    250d <= P <= 350d.
V1643 Sgr    Min II 12.1. According to [05771], RR?, P = 0.34d.
V1644 Sgr    The shape of the light curve varies.
V1647 Sgr    VB A (B 9.13m, 8", 104deg). Min II 7.43, DII = 0.059P,
             Min II - Min I = 0.262P (JD2441830);
             Min II = 2441830.55561 + 3.28282227d*E.
             The apsidal motion period is 592.5 +- 6.5 years.
V1648 Sgr    Close VB. Flat Min.
V1652 Sgr    Close VB. Flat Min.
V1653 Sgr    Close VB. Flat Min.
V1656 Sgr    Close VB. Flat Min.
V1658 Sgr    P var.Max = 2426560 + 105d*E (JD2417000 - 28000)
             [00842]; since JD2428000 - see Table.
V1660 Sgr    Close VB. Flat Min.
V1661 Sgr    Close VB. Flat Min. P var. Max = 2426850 + 275d*E
             (JD2424000 - 26850); since JD2436700 - see Table.
V1667 Sgr    P var. Max = 2426560 + 158d*E (JD2417000 - 36000)
             [00842]; since JD2436000 - see Table.
V1668 Sgr    Close VB. Flat Min.
V1670 Sgr    A var. P var. The shape of the light curve varies
             (probably with a period of about 11 years).
V1675 Sgr    A possible companion of 16m.
V1679 Sgr    Close VB. Flat Min.
V1681 Sgr    A possible companion of 16m.
V1690 Sgr    A possible companion of 16m.
V1691 Sgr    Close VB. Flat Min.
             P var. Max = 2426520 + 235d*E (JD2417000 - 28000)
             [00842]; since JD2436000 - see Table.
V1697 Sgr    A possible companion of 16m.
V1698 Sgr    A possible companion of 16m.
V1699 Sgr    P var. Max = 2425410 + 203.6d*E (JD2417000 - 27600)
             [00842]; since JD2436000 - see Table.
V1703 Sgr    A possible companion of 16m.
V1705 Sgr    P var. Max = 2425860 + 142d*E (JD2417000 - 27000)
             [00842]; since JD2435800 - see Table.
V1711 Sgr    [A/H] = -1.1. P var. Max = 2435365.19 + 30.46d*E
             (JD2432700 - 35400) [02570]; since JD2442200 - see Table.
V1714 Sgr    In the region of the open cluster Ruprecht 134.
V1721 Sgr    d = 0.03P:.
V1723 Sgr    Min II 13.8.
V1730 Sgr    Min II 14.8:; d = 0.03P:.
V1741 Sgr    In the nebula and the cluster NGC 6530 (M8). Var1.
V1743 Sgr    In the nebula and the cluster NGC 6530 (M8). Var2.
V1747 Sgr    In the nebula and the cluster NGC 6530 (M8). Var3.
V1748 Sgr    In the nebula and the cluster NGC 6530 (M8). Var4.
V1749 Sgr    In the nebula and the cluster NGC 6530 (M8). Var6.
V1750 Sgr    In the nebula and the cluster NGC 6530 (M8). Var8.
V1751 Sgr    In the nebula and the cluster NGC 6530 (M8). Var7.
V1752 Sgr    In the nebula and the cluster NGC 6530 (M8). Var13.
V1753 Sgr    In the nebula and the cluster NGC 6530 (M8). Var14.
V1755 Sgr    In the nebula and the cluster NGC 6530 (M8). Var15.
V1758 Sgr    In the nebula and the cluster NGC 6530 (M8). Var16.
V1761 Sgr    In the nebula and the cluster NGC 6530 (M8). Var19.
V1762 Sgr    In the nebula and the cluster NGC 6530 (M8). Var20.
V1764 Sgr    In the nebula and the cluster NGC 6530 (M8). Var23.
V1765 Sgr    In the nebula and the cluster NGC 6530 (M8). Var24.
V1768 Sgr    In the nebula and the cluster NGC 6530 (M8). Var26.
V1769 Sgr    In the nebula and the cluster NGC 6530 (M8). Var27.
V1771 Sgr    In the nebula and the cluster NGC 6530 (M8). Var29.
V1772 Sgr    In the nebula and the cluster NGC 6530 (M8). Var28.
V1773 Sgr    In the nebula and the cluster NGC 6530 (M8). Var31.
V1774 Sgr    In the nebula and the cluster NGC 6530 (M8). Var30.
V1775 Sgr    In the nebula and the cluster NGC 6530 (M8). Var33.
V1776 Sgr    In the nebula and the cluster NGC 6530 (M8). Var36.
V1777 Sgr    In the nebula and the cluster NGC 6530 (M8). Var37.
V1778 Sgr    In the nebula and the cluster NGC 6530 (M8). Var34.
V1779 Sgr    In the nebula and the cluster NGC 6530 (M8). Var40.
V1780 Sgr    In the nebula and the cluster NGC 6530 (M8). Var39.
V1781 Sgr    In the nebula and the cluster NGC 6530 (M8). Var41.
V1782 Sgr    In the nebula and the cluster NGC 6530 (M8). Var44.
V1784 Sgr    In the nebula and the cluster NGC 6530 (M8). Var45.
V1785 Sgr    In the nebula and the cluster NGC 6530 (M8). Var46.
V1786 Sgr    In the nebula and the cluster NGC 6530 (M8). Var48.
V1787 Sgr    In the nebula and the cluster NGC 6530 (M8). Var47.
V1788 Sgr    In the nebula and the cluster NGC 6530 (M8). Var50.
V1789 Sgr    In the nebula and the cluster NGC 6530 (M8). Var51.
V1790 Sgr    In the nebula and the cluster NGC 6530 (M8). Var49.
             Western component of a close pair.
V1791 Sgr    In the nebula and the cluster NGC 6530 (M8). Var53.
V1792 Sgr    In the nebula and the cluster NGC 6530 (M8). Var55.
V1793 Sgr    In the nebula and the cluster NGC 6530 (M8). Var54.
V1794 Sgr    In the nebula and the cluster NGC 6530 (M8). Var56.
V1795 Sgr    In the nebula and the cluster NGC 6530 (M8). Var58.
V1797 Sgr    In the nebula and the cluster NGC 6530 (M8). Var59.
V1798 Sgr    In the nebula and the cluster NGC 6530 (M8). Var60.
V1800 Sgr    In the nebula and the cluster NGC 6530 (M8). Var61.
V1801 Sgr    In the nebula and the cluster NGC 6530 (M8). Var62.
V1802 Sgr    In the nebula and the cluster NGC 6530 (M8). Var63.
V1803 Sgr    In the nebula and the cluster NGC 6530 (M8). Var64.
             SP component of a close pair.
V1805 Sgr    In the nebula and the cluster NGC 6530 (M8). Var66.
V1807 Sgr    In the nebula and the cluster NGC 6530 (M8). Var67.
V1808 Sgr    In the nebula and the cluster NGC 6530 (M8). Var68.
V1828 Sgr    P var. Max = 2424402 + 12.985d*E (JD2423800 - 36000)
             [02515]; since JD2436000 - see Table.
V1831 Sgr    P var. Max = 2428849.4 + 26.58d*E (JD2427500 - 31270)
             [02447]; since JD2435630 - see Table.
V1843 Sgr    P = 163.7d? [05869].
V1845 Sgr    Flat Min. Close companion?
V1864 Sgr    Epoch of light maximum is given.
V1869 Sgr    P var. Max = 2434178 + 346d*E (JD2427590 - 34220)
             [02447]; since JD2435630 - see Table.
V1882 Sgr    The shape of the light curve varies.
V1891 Sgr    A companion of 16m.
V1894 Sgr    V4 (NGC 6637). Possible member of the globular cluster
             NGC 6637 (M 69).
V1895 Sgr    P var. Max = 2421065 + 156.0d*E (JD2418850 - 21100);
             since JD2427600 - see Table.
V1900 Sgr    A companion of 15m.
V1904 Sgr    A companion of 15m.
V1911 Sgr    P var. Max = 2428832.4 + 10.0581d*E (JD2427600 - 34220)
             [02447]; since JD2435630 - see Table. The shape of the
             light curve varies?
V1925 Sgr    P var?
V1942 Sgr    In the region of the open cluster Ruprecht 147.
V1945 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6514 (M20).
V1946 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6514 (M20).
V1947 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6514 (M20). All the published charts
             for this variable are wrong. According to [09861] the
             star actually lies 1.1 mm south and 0.8 mm east of
             "D2" in fugure 3 published in [02428].
V1948 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6514 (M20).
V1949 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6514 (M20).
V1950 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6514 (M20).
V1951 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6514 (M20).
V1954 Sgr    VB(ro = 2"). P var.
             There is a nonlinear term in the elements:
             -4.1313d*10**(-8)*E**2.
V1958 Sgr    Min II 14.0.
V1962 Sgr    In the region of the open cluster and the
             diffuse nebula NGC 6618 (M 17).
V1963 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6618 (M 17).
V1966 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6618 (M 17).
V1969 Sgr    There are three close faint companions (15.8m-16.3m).
V1970 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6618 (M 17).
V1971 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6618 (M 17).
V1973 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6618 (M 17).
V1975 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6618 (M 17). The presence of a blue companion is
             possible.
V1976 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6618 (M 17).
V1977 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6618 (M 17).
V1980 Sgr    Min II 11.7; DII = 0.11P; Min II - Min I = 0.52P.
V1996 Sgr    VB.
V2003 Sgr    S 5.5/5. In the region of the open cluster M 25 (IC 4725).
V2007 Sgr    V 26 (NGC 6656 = M 22).
V2008 Sgr    P = 120 - 135d.
V2028 Sgr    In the region of the globular cluster NGC 6681 (M 70).
V2037 Sgr    A close companion is possible.
V2054 Sgr    P > 450d?
V2064 Sgr    VB. Combined brightness of the star and the close
             companion was estimated. It is not clear which star is
             variable.
V2065 Sgr    NP component of a close binary.
V2094 Sgr    P < 0.5d.
V2106 Sgr    VB. Combined brightness of the components was estimated.
V2148 Sgr    VB. Combined brightness of the components was estimated.
             The variable is the northern component.
V2276 Sgr    P < 30d.
V2282 Sgr    Star L. In the region of the open cluster and the diffuse
             nebula NGC 6514 (M20). Late spectrum.
V2283 Sgr    Min II 10.59:. Apsidal motion with P = 560 years [07107]:
             0.739P (1898) <= Min II - Min I <= 0.797P (1965).
             There are periodic terms in the
             elements given in the Table:
             +0.5414d*sin(0.006deg*(E + 45019)) - 0.0995d*sin(0.012deg*
             (E + 45019)) + 0.0217d*sin(0.018deg*(E + 45019)); Min II =
             2438946.7619 + 3.4714231d*E - 0.5414d*sin(0.006deg*
             (E + 45019)) - 0.0995d*sin(0.012deg*(E + 45019)) - 0.0217d*
             sin(0.018deg*(E + 45019)).
V2284 Sgr    P var.
V2285 Sgr    In the region of the globular cluster NGC 6558.
V2313 Sgr    Min II 16.8.
V2315 Sgr    P = 0.193d?
V2323 Sgr    Blue [08424].
V2341 Sgr    The epoch of Min brightness is given.
V2342 Sgr    V 17 (NGC 6626 = M28).
             The member of this globular cluster. Min II 13.5.
V2343 Sgr    A close companion of 14.5m.
V2346 Sgr    Cycles 50 - 100d.
V2349 Sgr    Min II 9.2.
V2351 Sgr    Min II 10.31.
V2352 Sgr    P var. There is a nonlinear term in the elements:
             0.0525d*E**2.
V2355 Sgr    In the region of the globular cluster NGC 6637 (M 69).
V2358 Sgr    In the region of the globular cluster NGC 6642.
V2359 Sgr    In the region of the globular cluster NGC 6637 (M 69).
V2360 Sgr    In the region of the globular cluster NGC 6637 (M 69).
V2361 Sgr    In the region of the globular cluster NGC 6637 (M 69).
V2362 Sgr    A close companion of 15m.
V2366 Sgr    P var. There is a nonlinear term in the elements:
             +0.6815d*10**(-9)*E**2.
V2367 Sgr    V28 (NGC 6656 = M22). Not a member of this globular cluster.
             P = 323d?
V2378 Sgr    Two close companions of 15.3m and 15.8m.
V2389 Sgr    P var?
V2391 Sgr    P = 189d?
V2413 Sgr    P var. The elements are valid in the interval
             JD2425440 - 30905.
V2416 Sgr    P.K. 7 +1G 2.
V2425 Sgr    E?
V2442 Sgr    P = 0.5d?
V2449 Sgr    Min II 17.4.
V2468 Sgr    Blue [08424].
V2471 Sgr    VB B (A 14.6m; B 8", 225deg).
V2493 Sgr    Blue [08424].
V2506 Sgr    P.K. 3 -4deg 6.
V2507 Sgr    Min II 14.6.
V2508 Sgr    Min II 14.1:.
V2509 Sgr    Min II 7.50.
V2510 Sgr    The epoch of Min brigtness is given. The elements given
             in the Table are valid since JD2427440.
V2520 Sgr    VB.
V2526 Sgr    The epoch of Min brightness is given.
             P var. Min = 2428699.5 + 31.3224d*E (JD2424100 - 31400)
             [05590]. Since JD2431400 - see Table.
V2529 Sgr    Min II 14.5. Twice shorter period is given in [05590].
V2540 Sgr    P var.
V2544 Sgr    VB?
V2552 Sgr    VB A (B 15.7m).
V2553 Sgr    There are two close companions.
V2562 Sgr    Northern component of a close pair. The companion is of
             16m.
V2563 Sgr    P var.
V2564 Sgr    P var?
V2565 Sgr    VB B (A 12.5m; B 90deg).
V2566 Sgr    P var. [Ca/H] = -0.52.
V2567 Sgr    [Ca/H] = -0.57.
V2568 Sgr    P var?
V2576 Sgr    P var. Max = 2426200 + 149d*E (JD2423500 - 27000);
             since JD2433000 - see Table.
V2577 Sgr    P var?
V2578 Sgr    VB. In the region of the globular cluster NGC 6642.
V2579 Sgr    P var. Max = 2429926.251 + 0.5911903d*E (JD2427590 -
             34200) [05590]; since JD2435600 - see Table.
V2584 Sgr    P var. Max = 2426564.347 + 0.534829d*E (JD2423940 -
             33860); since JD2437820 - see Table.
V2592 Sgr    In the region of the globular cluster NGC 6656 (M22).
V2593 Sgr    P var. Max = 2428780.349 + 0.5123825d*E
             (JD2427680 - 34200) [05590]; since JD2435600 - see Table.
V2594 Sgr    P var.
V2598 Sgr    A companion 15.8m. Spectrum description [06495].
V2601 Sgr    P.K. 12 -7deg 1.  The epoch of Min brightness is given.
V2616 Sgr    Min II 13.0.
V2617 Sgr    Min II 9.63.
V2620 Sgr    P = 185.6d?
V2625 Sgr    P = 0.75837d?
V2628 Sgr    P = 171d:?/205d:?/256d:?.
V2645 Sgr    P var?
V2649 Sgr    P = 143d:?
V2672 Sgr    P = 196.8d? /204.5d, /255.3d? /315.0d?
V2682 Sgr    P = 228.5d?
V2687 Sgr    P = 174d:?
V2703 Sgr    P = 270d:?
V2719 Sgr    SR?
V2731 Sgr    P = 147d:?
V2732 Sgr    P = 188.6d?
V2733 Sgr    P = 244d:?
V2736 Sgr    [Ca/H] = -1.45.
V2738 Sgr    [Ca/H] = -0.67.
V2740 Sgr    P = 269.0d?
V2745 Sgr    [Ca/H] = -1.15.
V2756 Sgr    P.K. 2 -5deg 1. The epoch of Min brightness is given.
V2763 Sgr    P = 216d:?
V2777 Sgr    [Ca/H] = -0.83.
V2783 Sgr    P = 265.0d?
V2789 Sgr    P = 255.5d?
V2798 Sgr    P = 244.5d?
V2816 Sgr    P = 250d:?
V2828 Sgr    P = 0.39669d?
V2830 Sgr    Cepheid?
V2833 Sgr    P = 224.0d?
V2834 Sgr    P = 275d:?
V2846 Sgr    P = 0.39659d?
V2868 Sgr    P = 235.5d?
V2876 Sgr    Min II 15.7:.
V2877 Sgr    P = 254.5d?
V2893 Sgr    P = 250d:?
V2900 Sgr    P = 0.49835d?
V2905 Sgr    Spectrum description [04452, 06495].
V2918 Sgr    P = 197d:?
V2937 Sgr    [Ca/H] = -0.75.
V2947 Sgr    RV Tau? Cepheid?
V2959 Sgr    P = 0.37233d?
V2962 Sgr    P = 209.5d?
V2967 Sgr    P = 0.68750d?
V2988 Sgr    P = 213.0d? The coordinates given in [05869] are erroneous.
V2996 Sgr    RV Tau? Cepheid?
V3004 Sgr    [Ca/H] = -0.76.
V3005 Sgr    RV Tau? Cepheid?
V3016 Sgr    P var?
V3032 Sgr    P = 153d:?
V3033 Sgr    The coordinates given in [05869] are erroneous.
V3034 Sgr    P = 154d:?
V3038 Sgr    P = 252d:?
V3052 Sgr    RV Tau? Cepheid?
V3062 Sgr    EW? P = 0.59610d?
V3065 Sgr    P = 179.8d?/215.5d?
V3071 Sgr    P = 291d:?
V3072 Sgr    P = 194d:?
V3088 Sgr    P = 215d:?
V3105 Sgr    [Ca/H] = -0.82.
V3106 Sgr    P = 261d:?
V3111 Sgr    P = 182.8d?
V3127 Sgr    UG? Not red.
V3128 Sgr    Nova? Only one Max was observed.
V3170 Sgr    [Ca/H] = -0.82.
V3175 Sgr    P = 179.8d?
V3176 Sgr    P = 197d:?
V3179 Sgr    P = 297d:?
V3186 Sgr    [Ca/H] = -1.28.
V3190 Sgr    P = 227.0d?
V3196 Sgr    RV Tau? Cepheid?
V3207 Sgr    P = 237d:?
V3239 Sgr    P = 226d:?
V3249 Sgr    UG?
V3285 Sgr    P = 173.8d /196.2d?
V3294 Sgr    P = 121d:? /177d:?
V3295 Sgr    P = 197d:?
V3335 Sgr    RV Tau? Cepheid?
V3353 Sgr    P var?
V3356 Sgr    P = 239.5d?
V3365 Sgr    P = 197d:? /252d:?
V3388 Sgr    P = 125d:? /160d:?
V3395 Sgr    P = 159d:?
V3412 Sgr    Cepheid?
V3433 Sgr    P = 287.0d?
V3443 Sgr    P = 177.6d?
V3444 Sgr    P = 160d:?
V3459 Sgr    P var. The shape of the light curve varies.
V3467 Sgr    RV Tau? Cepheid?
V3473 Sgr    SR?
V3500 Sgr    RV Tau? Cepheid?
V3501 Sgr    Min II 15.7:.
V3508 Sgr    The member of the open cluster M25 (IC 4725).
V3511 Sgr    RV Tau? Cepheid?
V3536 Sgr    P = 239.5d?
V3537 Sgr    P = 318.0d?
V3551 Sgr    P = 165.2d? /201.0d?
V3560 Sgr    P = 181d:?
V3564 Sgr    Cepheid?
V3566 Sgr    P = 249.0d?
V3583 Sgr    P = 228.0d?
V3588 Sgr    [Ca/H] = -0.69.
V3625 Sgr    P = 294d:?
V3634 Sgr    P = 145d:?
V3645 Sgr    In the region of the open cluster M25 (IC 4725).
V3709 Sgr    P = 240.0d?
V3718 Sgr    P var. There is a nonlinear term
             in the elements: +0.865d*10**(-10)*E**2.
V3748 Sgr    P = 0.305327d?
V3765 Sgr    [Ca/H] = -0.78.
V3783 Sgr    In the region of the globular cluster NGC 6681 (M70).
V3784 Sgr    P = 176.4d?
V3788 Sgr    In the region of the globular cluster NGC 6723. Red.
V3791 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6514 (M20).
V3792 Sgr    VB A (B 8.92m, 13.3", 90deg). Min II 6.81.
             The range of the combined light variation is given in the
             Table. The shape of the light curve varies.
V3804 Sgr    Spectrum description [06495, 07099].
V3811 Sgr    P2 = 4d? Spectrum description [07099, 09845].
V3817 Sgr    VB A (B 16m).
V3819 Sgr    P var. There is a nonlinear term in the elements:
             +10**(-10)*E**2.
V3829 Sgr    A close companion.
V3832 Sgr    A close companion.
V3834 Sgr    Cepheid or eclipsing?
V3837 Sgr    P = 0.565d? [06383].
V3838 Sgr    VB A (B 15.8m).
V3841 Sgr    P var. Max = 2431970 + 358d*E (JD2423900 - 33000);
             since JD2433000 - see Table.
V3842 Sgr    A close companion with M2? Spectral class possibly exists.
V3843 Sgr    In the region of the globular cluster NGC 6642.
V3853 Sgr    V22 (NGC 6656 = M22). The member of this globular cluster.
V3855 Sgr    V31 (NGC 6656 = M22). Possible member of the cluster.
V3857 Sgr    According to [06278] the spectral class is M8.
V3867 Sgr    Under the chart S 4903 is printed erroneously instead of
             CSV 4309.
V3868 Sgr    P var. Max = 2426130 + 270d*E (JD2423900 - 33900);
             since JD2435700 - see Table.
V3874 Sgr    P var. Max = 2436035 + 115.3d*E (JD2426000 - 38000);
             since JD2438000 - see Table.
V3875 Sgr    P var. P = 358d (JD2424000 - 33800); since
             JD2435000 - see Table.
V3876 Sgr    P var. Max = 2430090 + 345d*E (JD2423900 - 32000);
             Max = 2436830 + 358d*E (JD2436000 - 41500) [06279];
             since JD2441400 - see Table.
V3879 Sgr    VB (Delta(m) = 2.6m, ro = 0.6").
V3880 Sgr    OH, SiO, H2O maser.
V3885 Sgr    Porb = 0.206d [04939].
             Besides the irregular variability high-frequency
             oscillations are sometimes observed with
             P1 = 29.0s, P2 = 30.15s and with amplitudes of 0.00028m.
             In the spectrum there are extremely broad absorption
             lines of HI and HeI. The Balmer lines have emission
             components. X-ray source.
V3886 Sgr    Type EB?
V3893 Sgr    Connected with a ring nebula.
V3894 Sgr    Min II 6.37. P var?
V3899 Sgr    In the region of the open cluster and the diffuse nebula
             NGC 6514 (M20).
V3900 Sgr    V7 (NGC 6522). Not a member of this globular cluster.
V3903 Sgr    The member of the open cluster Collinder 367.
             In the nebula Simeis 188.
V3907 Sgr    The epoch of Min brightness is given.
V3929 Sgr    P.K.5 -5deg 2.
V3961 Sgr    SB1 (Porb = 690d [09915]).
V4024 Sgr    SB.
V4032 Sgr    Not far from V1309 Sgr.
V4034 Sgr    Flat Min. Close companion?
V4046 Sgr    Flares (11.1m - 12.4m U).
V4048 Sgr    Min II 12.6; DII = 0.15P.
V4051 Sgr    In the region of the globular cluster NGC 6638.
             Not a member of the cluster.
V4052 Sgr    In the region of the globular cluster NGC 6638.
             Not a member of the cluster.
V4054 Sgr    In the region of the globular cluster NGC 6638.
             Not a member of the cluster.
V4055 Sgr    In the region of the globular cluster NGC 6638.
             Not a member of the cluster.
V4058 Sgr    d = 0.02P
V4060 Sgr    P var. Max = 2437846 + 283d*E (JD2436030 - 38970);
             since JD2438970 - see Table.
V4066 Sgr    d ~0.07P.
V4067 Sgr    V32 (NGC 6656 = M22).
             Not a member of the globular cluster.
V4068 Sgr    V17 (NGC 6656 = M22).
             Not a member of the globular cluster.
V4069 Sgr    V33 (NGC 6656 = M22).
             Not a member of the globular cluster.
V4390 Sgr    SB2 and speckle binary.
V4417 Sgr    The variability may be due to the fainter (B) component.
V4429 Sgr    A giant, according to HIPPARCOS data, despite the published
             luminosity class (V).
V4955 Sgr    Close to the N of V4521 Sgr, the periods differ considerably.
V5099 Sgr    SU UMa-type cv.
V5112 Sgr    A symmetrical minimum lasted for several months, with variations also outside it.
eta   Sgr    VB A (B 8.0m, 3.5",105deg); mu alpha = -0.0107s,
             mu delta = -0.166".
mu    Sgr    VB A (B 10.48m, 16.9", 285deg; C 13.0m, 25.2", 119deg;
             D 9.69m, 48.5", 312deg; E 9.25m, 50.0", 115deg). SB2
             (e = 0.4). The variability type is EA/GS + ACYG.
             According to [09922] there are also quasiperiodical light
             variations with the amplitudes 0.08m - 0.15m and cycles
             from 16d to 40d.
ups   Sgr    Min II 4.59.
R     Sco    V7 (NGC 6093 = M80). Probable field star.
             P var. Max = 2400518 + 220.2d*E (JD2400500 - 04000)
             [00960]; Max = 2404493 + 225.86d*E (JD2404000 - 08600);
             Max = 2409003 + 222.29d*E (JD2408600 - 33300); since
             JD2433300 - see Table.
S     Sco    V6 (NGC 6093 = M80). Cluster non-member.
             P var. Max = 2400986 + 177.00d*E (JD2400900 - 17500);
             since JD2417500 - see Table.
T     Sco    4.0" N, 2.7" E from the center of the globular cluster
             NGC 6093 = M80.
U     Sco    Previous outbursts:
             2401646: (1863), 2417343 (1906), 2428342 (1936).
Y     Sco    Since 1972 varies its brightness in the range 12.3m-15.0m
             irregularly, maxima are unpredictable [08080].
Z     Sco    P var. Max = 2425546 + 357.17d*E (JD2412500 -
             25600); since JD2430000 - see Table.
RR    Sco    SiO maser. P var. Max = 2416944 + 284.31d*E
             (JD2411000 - 18000); Max = 2422828 + 278.09d*E
             (JD2422800 - 40000); since JD2440000 - see Table.
RU    Sco    P var. During JD2425000 - 40000 - see Table.
RV    Sco    VB A (B 13.0m, 5.9", 325deg).
RW    Sco    OH, H2O, SiO maser.
RY    Sco    P var, nonlinear term: +4.10d*10**(-6)*E**2. [A/H] = 0.2.
             VB A (B 10.70m, F8:, 13.8", 220.5deg, 1965;
             C 11.5m, 2.0", 102deg, 1964; D 11.43m, 24", 80deg).
             Combined brightness of AC is given.
RZ    Sco    P var. Max = 2413994 + 161.20d*E (JD2413600 - 22700);
             Max = 2422858 + 155.79d*E (JD2422700 - 28000);
             Max = 2428156  +  160.29d*E (JD2428000 - 35000); since
             JD2437500 - see Table.
SV    Sco    P var. Max = 2418886 + 258.5d:*E (JD2411600 - 19000);
             Max = 2424233 + 252.43d*E (JD2420500 - 28600);
             Max = 2429055 + 255.9d:*E (JD2428600 - 35000);
             since JD2437000 - see Table.
SY    Sco    In the region of the open cluster NGC 6475 = M7.
TX    Sco    In the region of the open cluster NGC 6475 = M7.
             Probable cluster member.
XX    Sco    The elements Max = 2413786 + 152d*E
             [00031] do not represent the observations from [09447].
AC    Sco    According to [00266], CST:, 12.2m - 12.6m pg.
AH    Sco    OH, H2O, SiO maser.
AI    Sco    P2 = 966.6d.
AL    Sco    Min II 11.3.
AN    Sco    EA type is possible.
AP    Sco    The chart in [09447] is wrong.
AR    Sco    According to [07104], T Tau type spectrum.
AU    Sco    VB A (B = V725 Sco, 0.4', 0deg).
AV    Sco    The chart and data in [09447] correspond to another star.
BI    Sco    VB B (A = GW Sco; B 6", 150deg).
BM    Sco    In the region of the open cluster NGC 6405 = M6.
BN    Sco    In the region of the open cluster NGC 6475 = M7.
             Resembles R Cen.
BS    Sco    d <= 0.03P. According to [00021], SP F8.
BT    Sco    P var. There is periodic term in the elements given in the
             Table: +0.05d*sin(176deg + 0.0857deg*E). Blazhko effect?
BV    Sco    Doubtful identification in [09447].
CF    Sco    Min II 13.8.
CK    Sco    VB A (B 15m, 14").
CL    Sco    The brightness in optical and UV range is modulated
             according to the elements: Min (pg) = 2427020 + 624.7d*E.
             Outbursts 1892, 1899, 1907, 1926.
CP    Sco    N /= 4.
CQ    Sco    [A/H] = -1.4.
DX    Sco    VB A (B p).
EZ    Sco    VB A (B 15.6m nf).
FQ    Sco    VB A (B 16m vis).
FU    Sco    VB A (B np). Min II 12.7, Min II - MiN I = 0.493P.
FV    Sco    d = 0.015P. Depth of Min II 0.1m pg.
FY    Sco    VB A (B 15m, 15", 35deg).
GG    Sco    VB A (B 15m, 8", 45deg).
GM    Sco    The nothern one of the two stars noted on the chart for
             SVS 1677.
GW    Sco    VB A (B = BI Sco, 6", 150deg).
IU    Sco    VB A (B 16.4m nf).
             Max = 2413280 + 69.05d*E (1893 - 1906);
             during 1910 - 1928 - see Table.
KO    Sco    Rapid variations: A = 1.0m. Slow changes:
             A = 0.5m, P = 2000d +-.
KQ    Sco    [A/H] = +0.3. P var?
LO    Sco    P var? Before JD2419150 Max = 2411500 + 450d*E;
             since JD2423900 - see Table.
             The spectrum is later than M5.
LR    Sco    The spectrum resembles RCrB in Max light [08090].
             IR excess. RCB type minima were not observed.
OO    Sco    In the region of the open cluster TR 29.
OQ    Sco    The chart in [06286] is wrong.
QZ    Sco    P var. Before JD2420400 Max = 2412640 + 158d*E;
             since JD2423900 - see Table.
V0347 Sco    P var. Before JD2418700 Max = 2411500 + 198d*E;
             since JD2423900 - see Table.
V0381 Sco    d = 0.046P.
V0382 Sco    In the region of the open cluster NGC 6475 = M7.
V0385 Sco    In the region of the open cluster CR 338.
V0387 Sco    Min II 12.2.
V0390 Sco    P var. Before JD2422500 Max = 2420330 + 466d*E;
             since JD2423900 - see Table.
V0393 Sco    Min II 8.3.
V0400 Sco    Min II 15.0.
V0402 Sco    In the region of the open cluster NGC 6475 = M7.
V0403 Sco    d ~0.02P. The depth of Min II 0.05m.
V0407 Sco    In the region of the open cluster NGC 6475 = M7.
V0411 Sco    Min II 14.0.
V0412 Sco    Min II 14.8. In the region of the open cluster
             NGC 6475 = M7.
V0420 Sco    In the region of the open cluster NGC 6475 = M7.
V0421 Sco    P var. Before JD2418000 Max = 2413830 + 293d*E;
             since JD2423900 - see Table.
V0423 Sco    Min II 14.2. In the region of the open cluster
             NGC 6475 = M7.
V0425 Sco    In the region of the open cluster NGC 6475 = M7.
V0426 Sco    In the region of the open cluster NGC 6475 = M7.
V0429 Sco    In the region of the open cluster NGC 6475 = M7.
V0430 Sco    In the region of the open cluster Tr 30.
V0432 Sco    In the region of the open cluster Tr 30.
V0437 Sco    d = 0.02P. Min II 13.9.
V0439 Sco    P var. Before JD2418200 Max = 2413350 + 166.5d*E;
             since JD2419900 - see Table.
V0440 Sco    In the region of the open cluster Tr 30.
V0446 Sco    P var? before JD2435000 Max = 2434980.1 +
             28.6195d. [A/H] = -1.0.
V0450 Sco    A = 0.9m pg.
V0453 Sco    VB A (B 13.51m, F7V, 13.5", 168deg). Min II 6.70.
             The light curve shape var?
V0455 Sco    P.K.351deg  + 3deg1. Planetary nebula nature is doubtful.
             Nova-like outbursts separated by several years.
V0457 Sco    Min II 11.3.
V0460 Sco    d = 0.02P.
V0464 Sco    d = 0.03P.
V0466 Sco    Min II 13.7.
V0467 Sco    P var. P = 2.41354d (1889 - 1903); since 1903 - see Table.
V0470 Sco    [A/H] = 0.1.
V0471 Sco    Min II 15.2, dII = 0.08P(!).
V0472 Sco    d = 0.02P.
V0474 Sco    Min II 10.6.
V0483 Sco    CI = +3.5m.
V0485 Sco    Short term variations are superimposed.
V0486 Sco    D >= 4d? P = 1d is possible. In the region of
             the open cluster NGC 6383.
V0487 Sco    [Fe/H] = -1.67, Delta(S) = 9.0.
V0490 Sco    Min II 12.5.
V0491 Sco    Min II 13.2.
V0494 Sco    A var (1.27m - 1.66m B). P var? Delta(S) = 2.
             VB A (B 12.72m y, 23").
V0495 Sco    Short term variation are superimposed.
             (Delta(m)short = 0.5m +-).
V0496 Sco    In the region of the open cluster NGC 6414.
             d = 0.03P.
V0497 Sco    Min II 13.6.
V0499 Sco    AII = 0.47m V. Min I - Min II = 0.504P.
V0502 Sco    In the region of the open cluster C 1712 - 407.
V0507 Sco    The epoch of Max from [00300] contradicts the elements.
V0540 Sco    VB A (B 15.2m sp).
V0547 Sco    VB B (A 14.2m sf).
V0549 Sco    [A/H] = -1.1.
V0555 Sco    [A/H] = -0.3.
V0562 Sco    Min II 12.1.
V0566 Sco    d = 0.01P:.
V0567 Sco    VB A (B 13.01m, 10"sp, CD 30"nf). P var.
V0568 Sco    d = 0.04P.
V0569 Sco    Min II 11.4.
V0570 Sco    P var? Unusually broad Max.
V0573 Sco    d = 0.06P. In the region of the open cluster Tr 24.
V0574 Sco    In the region of the open cluster Tr 24.
V0575 Sco    Min II 12.4.
V0579 Sco    In the region of the open cluster Tr 24.
V0581 Sco    Min II 11.9.
V0584 Sco    Min II 13.1.
V0585 Sco    d = 0.03P:.
V0586 Sco    d = 0.04P. In the region of the open cluster Tr 24.
V0588 Sco    d = 0.02P. In the region of the open cluster Tr 24.
V0589 Sco    d = 0.05P. In the region of the open cluster Tr 24.
V0590 Sco    In the region of the open cluster NGC 6231.
V0592 Sco    Min II 13.3.
V0593 Sco    d = 0.05P:.
V0594 Sco    d = 0.01P.
V0603 Sco    d = 0.04P.
V0606 Sco    d = 0.07P.
V0607 Sco    Min II 10.3.
V0609 Sco    Min II 13.7.
V0611 Sco    d = 0.04P. Min II 13.7.
V0612 Sco    d = 0.05P.
V0613 Sco    d = 0.04P.
V0616 Sco    Min II 12.4.
V0619 Sco    Min II 12.1.
V0620 Sco    d = 0.02P.
V0621 Sco    d = 0.04P.
V0622 Sco    Min II 14.2.
V0623 Sco    Long intervals in Max without changes, sometimes becomes
             faint.
V0625 Sco    VB A (B 13.2m sf). Min II 13.5.
V0627 Sco    Min II 14.1.
V0628 Sco    Min II 12.4.
V0629 Sco    Apsidal motion.
V0631 Sco    Min II 13.2.
V0632 Sco    d = 0.06P.
V0633 Sco    Min II 12.2.
V0634 Sco    Min II 12.2.
V0636 Sco    SB1 (Porb = 1318d).
V0638 Sco    d = 0.07P.
V0640 Sco    Min II 13.5.
V0656 Sco    The chart in [06286] is wrong.
V0660 Sco    VB A (B 16.0m s).
V0672 Sco    P = 180d is possible.
V0674 Sco    VB A (B 15.0m s).
V0677 Sco    The chart in [06286] is wrong.
V0679 Sco    P = 364d is possible.
V0690 Sco    VB A (B 14.40m y, 6", 0deg). The range of the combined
             light is given. Delta(S) = 4.
V0698 Sco    D <= 0.20d, d = 0.043d.
V0700 Sco    Min II 10.3.
V0701 Sco    Min II 9.05. P var. Min I = 2439329.6657 + 0.76187133d*E
             (JD2428000 - 39400) [07177]; since JD2439400 - see Table.
             Probable member of the open cluster NGC 6383.
V0702 Sco    Probable member of the open cluster NGC 6383.
V0703 Sco    P0 = 0.1499615d [03521]; P1 - see Table
             (P var?). Also noted P = 0.04162025d [03521].
             A var (0.23m - 0.46m). Beat phenomenon:
             Max = 2436760.249 + 0.497306d*E [03521]. Delta(S) = 1.
             In the region of the open cluster NGC 6405 = M6.
V0705 Sco    Min II 14.1:.
V0706 Sco    Moments of Max from [00046] contradict the tabulated
             elements. According to [04678], A <= 0.05m V
             during 6 nights.
V0708 Sco    In the region of the open cluster NGC 6475 = M7.
V0709 Sco    IN the region of the open cluster NGC 6475 = M7.
             [A/H] = -0.6.
V0710 Sco    Min II 14.2.
V0711 Sco    In the region of the open cluster NGC 6475 = M7.
V0712 Sco    Min II 14.0.
V0714 Sco    d = 0.05P:. P may be twice longer.
V0717 Sco    [A/H] = 0.9.
V0718 Sco    D ~4d. Another Min 2429847 - 849 [00270].
V0720 Sco    In the region of the open cluster NGC 6475 = M7.
V0723 Sco    In the region of the open cluster NGC 6475 = M7. At the
             edge of a dark cloud.
V0725 Sco    VB B (A = AU Sco, B 0.4', 0deg).
V0729 Sco    Possibly a Nova.
V0732 Sco    P may be twice longer.
V0733 Sco    Possibly a Nova.
V0734 Sco    Possibly a Nova.
V0735 Sco    The light curve shape var.
V0738 Sco    d = 0.04P:; Min II 13.4:. In the region of the open
             cluster NGC 6475 = M7.
V0740 Sco    In the region of the open cluster NGC 6475 = M7.
V0741 Sco    There is a red variable close to the coordinates in the
             discovery announcement [02448], but a different star is
             marked in the chart in [02448].
V0749 Sco    P = 410d is possible.
V0756 Sco    Min II 10.7.
V0760 Sco    dI = 0.02P; Min II 7.4; DII = 0.2P:, dII = 0.03P.
V0761 Sco    IN type is not excluded.
V0764 Sco    Min II 9.0.
V0805 Sco    Possibly P is twice shorter.
V0818 Sco    Sco X-1. SB.
             Var X-ray and multi-component radio source.
             Lx/Lbol = 300 - 1000. The epoch of Min is
             given for the periodic component of the light variation
             (A ~0.25m). Flickering and flares up to 1m with
             time scale from dozens of seconds to minutes. The
             mean brightness level decreased in the middle of
             1960-es by 0.3m-0.4m. The spectrum with blue continuum
             and H, HeI, HeII, CIII, NIII emissions.
V0819 Sco    Min II 13.2.
V0821 Sco    Min II 14.5.
V0822 Sco    VB? Combined brightness.
V0827 Sco    Min II 14.1.
V0833 Sco    Min II 11.2.
V0837 Sco    d ~0.03P:; Min II 14.3.
V0838 Sco    Min II 13.4.
V0842 Sco    Min II 12.3.
V0843 Sco    Min II 10.5.
V0848 Sco    Min II 13.1. RRC type with twice shorter period is
             possible.
V0849 Sco    Min II 14.1.
V0853 Sco    d = 0.05P; Min II 14.1.
V0856 Sco    VB C (A = BS 6000, 6.65m, AO-3III; B 12.55m, 16",
             298deg; C 44", 185deg; D 11.7m, CD 1.3", 105deg, 1945).
V0857 Sco    Erroneously labelled "10" (instead of "11") in the chart.
V0858 Sco    Erroneously labelled "11" (instead of "10") in the chart.
V0861 Sco    SB1. Min II 6.28. Depths of minima var. In the region of
             the open cluster NGC 6231, Cr 316, Tr 24.
V0862 Sco    Usually 6.67m - 6.76m. A flare of 40m duration on July 3,
             1965. In the region of the open cluster NGC 6405 = M6.
V0866 Sco    VB (Delta(m) ~0.5m, ~1", 200deg). m (6370 A) =
             11.14m - 12.37m. IR excess.
V0870 Sco    B-V =  +3.38m - +3.52m. In the region of the open cluster
             NGC 6231.
V0877 Sco    Min II 13.1.
V0883 Sco    VB A (B 12.60m, 9", 130deg). P var?
             Min = 2438228.315 + 1.294745d*E (JD2438200 - 40500)
             [06871]; since JD2440500 - see Table. Deep Min II.
V0884 Sco    4U 1700-37. LX/Lbol = 0.00007.
             Eclipsing X-ray source. Eclipse duration is variable
             in the ranges 0.61d <= dx <= 1.10d. The epoch of the
             middle of the X-ray eclipse coinciding with Min II is
             given. X-ray flux var in the scale from seconds till
             hours. Sometimes a periodic modulation with P ~97
             Min is present, its amplitude in the optical band reaches
             Delta(V) ~0.01m. Min II 6.57; Min I - Min II = 0.63P,
             dI=0.2P. Surrounded by the ring nebula Sh 2. in the region
             of the open cluster NGC 6281. Field star.
V0885 Sco    Noticeable Min II.
V0889 Sco    The northern component of a triple.
V0890 Sco    VB A (B 11.5m, 0.5' n).
V0894 Sco    A = 0.6m pg.
V0896 Sco    Co-ordinates or the chart may be erroneous.
V0900 Sco    In the region of the open cluster NGC 6231.
             The light curve is a sinusoidal wave. Possibly
             P = 6.20d; 6.85d.
V0903 Sco    N96 [02448]. Erroneously identified with V479 Sco.
V0906 Sco    In the region of the open cluster NGC 6475 = M7. Probable
             cluster member. VB (delta(mV) = 0.8m, 0.1", 111deg, 1957).
             The range of the combined light variation is given.
             Min II 6.21.
V0907 Sco    In the region of the open cluster NGC 6475 = M7.
             Min II 9.2.
V0911 Sco    Alternative P = 4.2d.
V0913 Sco    Alternative P = 0.976d. IR excess.
V0914 Sco    VB (delta(mV) = 2m, 3", 200deg). Sine wave with P = 2.69d,
             Delta(B) = 0.15m (B = 12.91m) [09753].
V0915 Sco    VB A (B 10.43m, WN6, 14", 330deg; C 11.40m, 20", 202deg;
             D 13.96m, 22", 80deg, 1973). The brightness decreased from
             6.32m to 6.50m during JD2443680 - 44115.
V0917 Sco    VB A (B 17m: sp). The outburst: rise 1930-1936,
             Max 1936-1938, decline 1938-1952.
V0919 Sco    In the region of the open cluster NGC 6231.
V0920 Sco    In the region of the open cluster NGC 6231. Multiple
             periodicity: P1 - see Table, semiamplitude A1 = 0.0051m;
             P2 = 0.10765d. A2 = 0.0046m; P3 = 0.10388d, A3 = 0.00485m;
             P4 = 0.12137d, A4 = 0.0036m; P5 = 0.6929d?, A5 = 0.0028m.
V0921 Sco    The star illuminates a nebula.
V0922 Sco    Multiple periodicity, superposition of frequencies with
             amplitudes 0.0010m - 0.0352m.
V0923 Sco    D = 0.32d:. The elements need confirmation. In the region
             of the open cluster NGC 6281.
V0924 Sco    B-V var: +1.90, +2.50,
             Light fluctuations by 0.1m - 0.2m (u, b) in several
             minutes.
V0925 Sco    VB A (B ~10", faint, blue). Probable member of the open
             cluster TR 27. In Vr possible values of P: 105.3d, 73.0d,
             188.7d, 312.5d [09950].
V0926 Sco    3U 1735-44 = Sco XR-3. Bursts superimpose small light
             variations with P = 0.18d which is apparently the
             orbital period [04394].
V0927 Sco    The epoch of Min in U light is given. IR excess.
alf   Sco    ADS 10074 A(B 5.1m, B4Ve, A = 2.9", Porb = 878 yr.).
             Connected with a nebula.
zet 1 Sco    In the region of the open cluster NGC 6231.
kap   Sco    SB. P2 = 0.205430d. P1 var. Beat phenomenon:
             Pi = 7.3316d.
lam   Sco    SB1. Porb = 5.6d? Apuls = 0.02m. Long period light changes:
             Max = 2440376.15 + 10.1605d*E [09761]. One eclipse was
             found (JD2440690, A ~0.04m) [06388].
mu  1 Sco    Min II 3.12.
sig   Sco    VB AA (A 5.5m, 0.37", 96deg, 1981,
             orbital motion?; B 8.45m, B9.5V, 20.1", 273deg,
             1961); SB1, Porb = 33.06d. P0 var.
             Max Vr = 2420000.1465 + 0.24682815d*E (1918 - 1924)
             [09953]; Max = 2432306.918 + 0.246846d*E (JD2432000 - 37800)
             [09764]; since JD2437800 - see Table.
             A0 = 0.036m y. P1 = 0.2396674d, A1 = 0.013m y [09762].
             Pbeat = 8.256d = Porb/4 [09957].
             Connected with a nebula.
R     Scl    VB A (B 19.9m, 10", 234deg). CO emission.
S     Scl    P var. Max = 412774 + 367.9d*E (JD2405400 - 20500);
             Max = 2423035 + 360.6d*E (JD2421250 - 27740);
             Max = 2427738 + 370.4d*E (JD2427700 - 34000) [00960];
             Since JD2434000 - see Table. H2O emission.
T     Scl    P var. Max = 2417400 + 202.26d*E (JD2411300 - 19000);
             Max = 2420390 + 197.85d*E (JD2419000 - 23600);
             since JD2423600 - see Table.
V     Scl    P var. Max = 2414006 + 294.8d*E (JD2411600 - 18200);
             Max = 2422866 + 297.2d*E (JD2420400 - 35100);
             since JD2435100 - see Table.
X     Scl    P var. Max = 2413796 + 258.7d*E (JD2413500 - 22800);
             since JD2422800 - see Table.
Y     Scl    The cycles 100d: and 300d: are sometimes observed.
RT    Scl    Min II 10.47. [Fe/H] = -0.75. P var. There is
             a nonlinear term in the elements given in the Table:
             -9.04d*10**(-11)*E**2.
RU    Scl    (k - b)2 = 0.09. A var [03429]. P var. Max = 2425094.4175 +
             0.4933257d*E (JD2416750 - 25100) [00183]; Max =
             2427403.177 + 0.4933239d*E (JD2425100 - 30650)
             [01381]; since JD2430650 - see Table.
RW    Scl    P var?
SV    Scl    [Fe/H] = -1.82. P var? Max = 2439468.364 +
             0.3773636d*E (JD2427300 - 39500) [05233];
             since JD2439850 - see Table.
SY    Scl    H2O maser. P var? Max = 2426160 + 411d*E [00193]; since
             JD2440400 - see Table.
SZ    Scl    Min II 13.68.
UY    Scl    Near the galaxy NGC 55.
UZ    Scl    VB A (B 15.81m, 23", 135deg); (k - b)2 = 0.14. The
             shape of the light curve varies.
VV    Scl    Min II 8.50. ACV? [08083].
VY    Scl    Porb = 0.1662d? [09932]. High and low states of the
             system are observed.
VZ    Scl    High and low states of the system are observed [09933].
WZ    Scl    There are two oscillations with the periods P1 and
             P2: P1 = 0.06576d, P2 = 0.095944d, P1/P2 = 0.6854.
XX    Scl    There are two oscillations with the periods P1 and
             P2: P1 = 0.048898d, P2 = 0.051350d, P1/P2 = 0.95225.
AI    Scl    There are two oscillations with the periods P1 and
             P2: P1 = 0.044d, P2 = 0.0931d, P1/P2 = 0.47.
AL    Scl    Min II 6.20; Min II - Min I = 0.475P; DII = 0.08P.
AO    Scl    mu = 0.46", P = 187deg.
BC    Scl    May be eclipsing.
BI    Scl    Type E: is also possible.
R     Sct    [Fe/H] = -1. P var. Min I = 2377165 + 142.8d*E
             (JD2377160 - 9820); Min I = 2384885 + 142.6d*E
             (JD2384890 - 8170); Min I = 2394451 + 141.4d*E
             (JD2394450 - 8500); Min I = 2398777 + 142.4d*E
             (JD2398770 - 2404320); Min I = 2404627 + 137.4d*E
             (JD2404600 - 6410); Min I = 2406561 + 142.7d*E
             (JD2406560 - 9065); Min I = 2409742 + 143.6d*E
             (JD2409730 - 12700); Min I = 2412755 + 141.5d*E
             (JD2412750 - 16720); Min I = 2417161 + 139.5d*E
             (JD2417150 - 20790); Min I = 2421083 + 143.4d*E
             (JD2421050 - 25170) [09935]; Min I = 2429478 + 142.8d*E
             (JD2429000 - 30650) [09938]; Min I = 2432078 + 140.05d*E
             (JD2432000 - 42240) [07596]; Min I = 2442737 + 152.5d*E
             (JD2442550 - 43050); Min I = 2443315 + 138.5d*E
             (JD2443050 - 44150) [00001]; since JD2444150 - see Table.
             Light curve drawings [09935, 09936, 9937].
             Spectrum description [09939, 09954].
S     Sct    VB A (B 11.9M V, 14.5", 238deg; C 12.5m V, 44", 105deg).
U     Sct    Min II 10.31.
W     Sct    Min II 10.1.
X     Sct    [A/H] = -0.1. In the region of the open cluster NGC 6639.
Y     Sct    In the region of the open cluster NGC 6664.
Z     Sct    [A/H] = 0.3.
RS    Sct    Min II 10.08.
RU    Sct    [A/H] = -0.7. P var. There is a nonlinear term in the
             elements given in the Table: +3.15d*10**(-6)*E**2.
RX    Sct    Connected with the bright hydrogen nebula YM 13.
RY    Sct    Min II 9.56. P var? Min I = 2427979.340 + 11.124939d*E
             (JD2414800 - 36100) [00007]; since JD2431200 - see Table.
             The shape of the light curve varies.
RZ    Sct    Min II 7.47. P var. There is nonlinear term in the
             elements given in the Table: +0.78d*10**(-7)*E**2.
SU    Sct    P var. Max = 2424324.48 + 1.467713d*E (JD2420700 - 34310);
             Max = 2439678.428 + 1.468753d*E (JD2437100 - 41100) [07806];
             since JD2441100 - see Table.
TX    Sct    CWA? red.
TY    Sct    [A/H] = -0.3. In the region of the open cluster Tr 35.
UZ    Sct    [Fe/H] = 0.35. P var. Max = 2435629.5 + 14.7468d*E
             (JD2423900 - 35700) [02309]; since JD2436000 - see Table.
VV    Sct    SF component of a pair.
VW    Sct    P var. Max = 2415887 + 234d*E (JD2411900 - 22210);
             Max = 2423588 + 235d*E (JD2422880 - 27600);
             Max = 2429468 + 235.1d*E (JD2428750 - 34200);
             since JD2434600 - see Table.
VX    Sct    d = 0.064P.
VZ    Sct    Min II 12.0.
WY    Sct    P var.
XY    Sct    Min II 14.5.
AC    Sct    d = 0.024P; Min II 10.2.
AE    Sct    d = 0.04P.
AI    Sct    In the region of the open cluster NGC 6705.
AN    Sct    P var?
AP    Sct    V2 (NGC 6712).
AU    Sct    d ~0.03P.
BC    Sct    Following component of a close double system. The
             companion - NSV 11551.
BH    Sct    Min II 14.9.
BI    Sct    VB A (B 16.3m:, 3", 280deg; C 16.7m:, 12", 190deg;
             D 16.8m:, 18", 45deg; E 17.0m:, 6", 350deg).
BK    Sct    Close companion 16.5m sf.
BN    Sct    d = 0.02P.
BP    Sct    S 5.5/5.5.
BS    Sct    Min II 11.07. In the region of the open cluster M11
             (NGC 6705).
BU    Sct    A var. P var. Max = 2425804.625 + 0.42022d*E [01401];
             Max = 2427928.041 + 0.4202188d*E (JD2427900 - 9440)
             [01404]; Max = 2432770.464 + 0.4201944d*E
             (JD2432740 - 38290); Max = 2438589.357 + 0.4202171d*E
             (JD2438580 - 40510) [07806]; since JD2440770 - see Table.
BX    Sct    [A/H] = -0.9.
CD    Sct    Min II 13.7.
CF    Sct    d = 0.035P.
CH    Sct    V7 (NGC 6712). The member of this globular cluster.
CK    Sct    [Fe/H] = 0.23.
CL    Sct    May be the period should be doubled?
CM    Sct    [A/H] = 0.1.
CN    Sct    [A/H] = -1.5.
CO    Sct    P var? Resembles RV Tau type variables: if the period is
             doubled, the neight of max I and the depth of Min II vary.
CR    Sct    Min II 12.1; DII = 0.071P; Min II - Min I = 0.53P.
CT    Sct    Min II 11.1.
CW    Sct    Min II 10.1.
CZ    Sct    The epoch of Min brightness is given.
DD    Sct    One of the components probably varies.
DE    Sct    Min II 16.3.
DG    Sct    d = 0.03P:.
DL    Sct    Min II 15.9.
DT    Sct    Min II 16.5.
DV    Sct    Min II 17.8.
DW    Sct    Min II 16.4.
EE    Sct    Min II 15.3.
EH    Sct    Min II 15.0.
EK    Sct    Min II 16.0.
EL    Sct    The shape of the light curve varies?
EN    Sct    Min II 17.2. The different elements are also possible:
             Min I = 2428008.85 + 1.06446d*E.
EP    Sct    d = 0.04P:; Min II 15.6.
EQ    Sct    In the region of the open cluster NGC 6631. Min II 12.6:.
ER    Sct    Min II 9.3; Min II - Min I = 0.506P; DII = 0.14P.
EU    Sct    VB A (B 17.5m, 6", 45deg).
EV    Sct    [A/H] = -0.4. The member of the open cluster NGC 6664.
EW    Sct    P0 = 5.8195d (A/2 = 0.27m), P1 = 4.0646d (A/2 = 0.22m);
             P1/P0 = 0.6984.
EX    Sct    d = 0.025P:.
EY    Sct    Min II 12.4. In the region of the open cluster NGC 6683.
EZ    Sct    Min II 12.5.
FF    Sct    Min II 14.2.
FG    Sct    Min II 14.70. P var? Min I = 2429017.557 + 0.2705728d*E
             (JD2427975 - 29520) [01397]; since JD2444700 - see Table.
FH    Sct    In the region of the open cluster NGC 6694.
FK    Sct    Min II 14.4:.
FL    Sct    Min II 13.8.
FM    Sct    Min II 12.9.
FN    Sct    In the open cluster NGC 6704.
FO    Sct    D = 0.22d.
FR    Sct    Spectrum description [01410].
GI    Sct    Min II 14.5.
GM    Sct    Min II 13.8:.
HI    Sct    D = 0.29d.
HL    Sct    Min II 13.4.
IS    Sct    P < 200d.
IT    Sct    In the region of the open cluster NGC 6705.
LL    Sct    sf component of a close pair.
LR    Sct    In the region of the globular cluster NGC 6712.
LU    Sct    P2 = 30d.
LZ    Sct    In the region of the globular cluster NGC 6712.
MM    Sct    Min II 15.8.
MP    Sct    V1 (NGC 6712). The member of this globular cluster.
             [Fe/H] = -0.69.
MR    Sct    V8 (NGC 6712). P var. Max = 2430885 + 117d*E
             (JD2427900 - 32400) [04231]; since JD2434900 - see Table.
NU    Sct    VB A (B 16.6m, 12", 180deg).
NV    Sct    P = 200d?
OU    Sct    P var. Max = 2427620 + 152d*E (JD2426200 - 32800);
             since JD2433100 - see Table.
PT    Sct    There is a close companion, 16.4m.
PW    Sct    The range of the combined light of the variable and
             a close companion, which follows, is given in the Table.
QU    Sct    The variable is also eclipsing one with P = 0.2d and
             A = 0.7m.
V0337 Sct    A close companion (16.2m, <7", 90deg).
V0340 Sct    Min II 15.6.
V0356 Sct    Min II 12.3; DII = 0.10P.
V0360 Sct    A close fn companion, 16.4m.
V0362 Sct    P = 170d?
V0367 Sct    In the open cluster NGC 6649. The light elements
             with fundamental mode period P0 (A0 = 0.54m B) are
             given in the Table. For the first-overtone period
             P1 (A1 = 0.41m B) Max = 2437435.12 + 4.38466d*E;
             P1/P0 = 0.696744. M - m var (0.15 <= M - m <= 0.45).
V0369 Sct    In the region of the open cluster NGC 6705 (M 11).
             There is a superposition of the four light oscillations:
             P1 = 0.240d (A1 = 0.044m), P2 = 0.220d (A2 = 0.020m),
             P3 = 0.182d (A3 = 0.068m), P4 = 0.114d (A4 = 0.028m)
             [09745].
V0370 Sct    d = 0.016P.
V0372 Sct    d = 0.012P.
V0414 Sct    Blue companion?
del   Sct    VB A (B 10m, 53", 130deg); (k - b)2 = 0.37.
             The basic light variation P0 (A0 = 0.125m) given in the
             Table is superposed by the secondary one with
             P1 = 0.1867756 (A1 = 0.034) [09975].
R     Ser    P var. Max = 2372429 + 356.93d*E (JD2372400 - 88900)
             [00960]; Max = 2397809 + 353.00d*E
             (JD2394000 - 2403000); Max = 2403104 + 357.25d*E
             (JD2403000 - 24000); Max = 2432387 + 356.10D*E
             (JD2424000-39200); since JD2441000 - see Table.
             Maser (SiO, H2O).
S     Ser    P var. Max = 2394360 + 361.01d*E (JD2394000 - 2407000);
             Max = 2407024 + 372.70d*E (JD2407000 - 17000) [00960];
             Max = 2425875 + 366.59d*E (JD2417000 - 36000); since
             JD2437600 - see Table. Maser (OH, SiO, H2O).
T     Ser    In the region of the open cluster NGC 6633.
             P var. Max = 2400907 + 342.05d*E (JD2400500 - 15000);
             Max = 2417912 + 345.73d*E (JD2417900 - 26000);
             Max = 2428524 + 332.21d*E (JD2426000 - 32500);
             Max = 2438382 + 345.71d*E (JD2432500 - 39500); since
             JD2439500 - see Table. 0.8' from BN Ser.
U     Ser    P var. Max = 2421158 + 237.70d*E (JD2414000 - 22000);
             Max = 2422347 + 236.78d*E (JD2422000 - 26600);
             Max = 2426609 + 239.21d*E (JD2426600 - 32500);
             since JD2432500 - see Table.
V     Ser    Min II 9.85.
W     Ser    P var, nonlinear terms:
             +(3.140d*10**(-6))*E**2 + (1.432d*10**(-9))*E**3.
             The light curve shape var. Wavelike variations in Max
             light. Changes of emission lines with the orbital phase.
             Active mass exchange, evidence for a common envelope.
X     Ser    After 1932 variations 14.3m - 18.3m were noted; according
             to [01417], P = 275d. Observations in 1961 - 1964 did not
             confirm P = 275d, fluctuations of light with a period of
             several minutes were suspected [03625]. The spectral data
             are for 1981.
Y     Ser    Epoch of min is given. According to [08643], variations
             with P ~400d are superimposed by P ~40d.
Z     Ser    The elements are valid during JD2422000 - 31000.
RS    Ser    Min II 11.4.
RT    Ser    Max (1920 - 1923). In the spectrum (1977 - 1979) there are
             emissions Halpha - Hdelta, HeI, HeII, [OI] etc.
             Absorptions TiO.
RV    Ser    Maser (H2O).
VY    Ser    [Fe/H] = -1.77, Delta(S) = 9.
WW    Ser    Maser (H2O).
WX    Ser    Maser (OH, SiO, H2O). P var?
AA    Ser    [A/H] = 0.2.
AG    Ser    P var? since JD2435000 - see Table.
AK    Ser    P var? before JD2442300 Min = 2431313.266 + 1.9225667d*E
             [00318]; since JD2442300 - see Table.
AN    Ser    P var? Max = 2429156.260 + 0.5220703d*E
             (JD2427000 - 38000) [00001]; since JD2438000 - see Table.
             According to [02740], Blazhko effect with Pi = 21.94d;
             the presence of the Blazhko effect is denied in [07258].
             Delta(S) = 0.
AO    Ser    Min II 10.8.
AP    Ser    VB A (B 14.29m, 8" sp). [Fe/H] = -1.37.
AQ    Ser    Min II 11.1.
AR    Ser    P var. Before JD2425000 Max = 2415617.698 + 0.5752221d*E;
             Max = 2425313.530 + 0.57508945d*E
             (JD2425000 - 28500); Max = 2428848.662 + 0.575214d*E
             (JD2428500 - 31000) [08081]; Max =
             2431436.424 + 0.5751134d*E (JD2431000 - 34200);
             Max = 2436013.279 + 0.5752169d*E (JD2435900 - 37200);
             Max = 2438138.467 + 0.5750651d*E (JD2437200 - 38700)
             [00001]. Elements working on average since JD2438700 - see
             Table. Complex Blazhko effect. Pi = 108.4d [08082].
             A var (0.23m - 0.87m V). Pi var (80d - 120d) [07032].
             Delta(S) = 4.6.
AS    Ser    Min II 11.5. The epoch of Min I 2442937.428
             (BBSAG) is not in agreement with the elements.
AT    Ser    P var. Max = 2415353.783 + 0.74655695d*E
             (JD2415000 - 27000); Max = 2428337.260 + 0.7465670d*E
             (JD2428000 - 39500); since JD2441500 - see Table.
             Delta(S) = 9.
AU    Ser    Min II 11.61.
             The light curve shape var.
AV    Ser    Delta(S) = 6.
AW    Ser    Delta(S) = 5.0.
BF    Ser    [A/H] = -2.5. Delta(S) = 6.
BH    Ser    P var. Max = 2427956.674 + 0.434545d*E (JD2425000 -
             30700) [01039]; since JD2437650 - see Table.
BI    Ser    Min I 2446264.414 [10200] contradicts the elements. P var?
BN    Ser    In the region of the open cluster NGC 6633. 0.8' from
             T Ser.
BO    Ser    P var? Max = 2425681 + 201d (JD2425600 - 30100)  0447];
             the Table gives mean elements (JD2425600 - 35400).
BQ    Ser    P0 - see Table. P1 = 3.012d [08188]. In the region of the
             open cluster IC 4756.
BR    Ser    In the region of the open cluster IC 4756.
BS    Ser    In the region of the open cluster IC 4756.
BT    Ser    In the region of the open cluster IC 4756.
BU    Ser    In the region of the open cluster IC 4756.
CC    Ser    Min II 11.63.
CN    Ser    [Fe/H] = -0.77. Delta(S) = 3.4.
CO    Ser    P var? The light curve shape var.
             [Fe/H] = -1.38. Delta(S) = 7.2.
CQ    Ser    Min II 12.0.
CR    Ser    [A/H] = -0.2.
CS    Ser    P var. Max = 2418137.875 + 0.5267904d*E
             (JD2416000 - 32500) [00001]; since JD2432500 - see Table.
             Delta(S) = (6). In the region of the HII complex S 54 and
             the open star cluster NGC 6604. Connected with a
             shell-structure nebula. Sometimes eclipses are observed
             during the configuration "WR in front of O" (see Table)
             and sometimes during the configuration "O in front of
             WR" which coincided with the deepest eclipse ever observed
             (with the depth 0.5m B, V). Sometimes the photometric
             eclipse at predicted moments does not occur, and only the
             atmospheric eclipse of the O star with the WR component is
             observed at lambda 4653 A (emission of CII - CIV, NIII),
             lambda < 2000 A. IR excess; possibly an IR eclipse in
             the configuration "O  in front of WR".
CX    Ser    The light curve (resembling the eclipsing light curve of
             U Gem) shows a hump of ~0.2m height before the minimum;
             fluctuations up to ~0.3m - 0.4m in Max.
DF    Ser    VB A (B 13.9m, 0.4', -115deg).
DG    Ser    Min II 16.5:. The alias period is possible (0.3360742d).
DH    Ser    Another possible P = 450d.
DK    Ser    Max 2433829 [10008] contradicts the elements.
DR    Ser    VB A (B 12.54m, 28", 0deg).
DT    Ser    VB A (B ~5"). The spectrum shows emissions of [OIII]
             lambda lambda 4959, 5007 A. Symbiotic? [08676].
DV    Ser    In a small star cluster.
DY    Ser    [Fe/H] = -1.58. Delta(S) = 8.4.
EE    Ser    In the region of the open cluster M 17 = NGC 6618.
EF    Ser    In the region of the open cluster M 17 = NGC 6618.
EG    Ser    VB A (ro > 10").
EL    Ser    N <= 7.
EN    Ser    [Fe/H] = -1.07. Delta(S) = 5.3.
EO    Ser    The light curve shows large scatter. RR(B) type is
             possible. Max = 2437433.653 + 0.6309d*E (JD2437433 - 514)
             [3625]. [Fe/H] = -1.63. Delta(S) = 8.8.
ER    Ser    In the region of the open cluster M 16 = NGC 6611.
ES    Ser    In the region of the open cluster M 16 = NGC 6611.
ET    Ser    In the region of the open cluster M 16 = NGC 6611.
EU    Ser    VB A (B 4" np). A member of the open cluster
             M 16 = NGC 6611. IR excess.
EV    Ser    In the region of the open cluster M 16 = NGC 6611.
EW    Ser    In the region of the open cluster M 16 = NGC 6611.
EX    Ser    In the region of the open cluster M 16 = NGC 6611.
FI    Ser    Hints of periodicity in U light.
FK    Ser    VB (Delta(m) ~0.5m, 1.3", 11.5deg, 1972).
             Flares were found in the satellite UV range [10013].
             Differences from typical by stars and probable "post-T Tau"
             nature are noted [07260, 03866]. According to [06948],
             Min = 2441939.200 + 5.20d*E. Soft X-ray source.
FL    Ser    VB (Delta(m) = 1.9m, 0.46", 145deg, 1981).
FM    Ser    In the region of the open cluster M 16 = NGC 6611.
             VB (var sf?).
FN    Ser    In the region of the open cluster M 16 = NGC 6611.
FR    Ser    ADS 11477 A (B 12.5m, 10.5", 330deg, 1924; C 9.3m,
             30.5", 5deg, 1930). Possible values of P: 2.1308d, 2.1565d.
LN    Ser    m pg ~17.5m ~const; blue companion? [07264].
LS    Ser    The light curve shows large scatter, the elements need
             confirmation. Possible identification with an X-ray source
             2ASE 1822 + 0.
LV    Ser    The epoch of max in V light is given; in B and U varies
             in opposite phase.
LX    Ser    The depth of eclipses ~2.5m. Comparatively frequent
             outbursts [10023].
MM    Ser    Ser X-1 = 4 U 1 837 + 04. LX/Lopt >= 100.
             VB B (A 19.1m; B 2.2", 210deg).
MO    Ser    V1 (NGC 6535). Cluster non-member.
MP    Ser    V2 (NGC 6535). Cluster non-member.
OU    Ser    SB2.
PS    Ser    Both components are SB systems, Porb(A) = 15.888d,
             Porb(B) = 13.561d.
PT    Ser    SB, Porb = 38.937d.
del   Ser    ADS 9701A (B 5.16m, dF0, a = 5.843", Porb = 3168 yr;
             4", 175G, 1980).
omi   Ser    SB?
d     Ser    ADS 11353 A (B 7.44m, SB?, F5V, 3.9", 320deg, 1983).
             VB (speckle-interferometric; 0.25", 157deg, 1976).
             SB (P1orb = 385d, P2orb = 1.8505205d).
S     Sex    P var. Max = 2422029 + 257.2d*E (JD2417650 - 22050);
             Max = 2428968 + 266.65d*E (JD2422050 - 30300); Max =
             2434739 + 260.86d*E (JD2430300 - 34750); Max =
             2438796 + 254.3d*E (JD2434750 - 38800);
             since JD2440600 - see Table.
T     Sex    [Fe/H] = -1.20. P var. Max = 2416146.675 + 0.32465971d*E
             (JD2414000 - 18300), Max = 2424561.398 + 0.32467107d*E
             (JD2418300 - 24570) [00752];
             Max = 2424561.430 + 0.3246702d*E (JD2424560 - 28280),
             Max = 2429350.320 + 0.3247113d*E (JD2429350 - 34370),
             Max = 2434795.409 + 0.3246978d*E (JD2434795 - 36630)
             [09978]; since JD2441380 - see Table.
U     Sex    P var. Max = 2419823.355 + 0.53402622d*E
             (JD2419470 - 36670) [03697]; since JD2443980 - see Table.
Y     Sex    Min II 10.17; dII = 0.05P. P var. Min I = 2428122.700 +
             0.41982341d*E (JD < 2429000) [00007]; Min I =
             2434445.989 + 0.419818d*E (JD2428100 - 35000)
             [00001], Min I = 2439521.964 + 0.41981543d*E
             (JD2431150 - 43250) [09981]; since JD2440300 - see Table.
RU    Sex    Min II 11.4. According to [09923], RR?
             (P = 0.5398d?), CEP? (P = 6.792d?).
RW    Sex    Porb = 0.247d [09925]; LX/Lopt = 10**(-4) [09926];
             Px = 254s [09927].
RX    Sex    VB A (B 9.1m, 116.3", 191deg).
RY    Sex    Mu = 0.67", P = 281deg.
R     Tau    OH, H2O, Sio maser. P var. Max = 2411012 +
             325.0d*E (JD2398654 - 2414000); Max = 2424243 +
             322.1d*E (JD2414000 - 24300); Max = 2434005 +
             325.4d*E (JD2424300 - 35500); since JD2435500 - see Table.
S     Tau    P var. Max = 2404646 + 380.1d*E (JD2399326 - 2405000);
             Max = 2425085 + 371.40d*E (JD2405000 - 26000); since
             JD2426000 - see Table.
T     Tau    VB A (B 15m, 0.27", 358deg; C - infrared companion, 0.590",
             180deg). Near the variable nebula NGC 1555. OH, H2O maser.
             In the interval JD2402140 - 21000 the light range
             9.3m - 13.5m, since JD2421000 - only 9.5m - 10.8m.
U     Tau    VB (A 10.9m; B 12.0m, 3", 77deg).
V     Tau    P var. Max = 2417978 + 170.0d*E (JD2404550 - 18000);
             Max = 2424580 + 169.3d*E (JD2418000 - 24600);
             Max = 2432746 + 170.1d*E (JD2424600 - 33500);
             Max = 2436970 + 168.7d*E (JD2433500 - 37300);
             Max = 2442442 + 171.1d*E (JD2437300 - 43000);
             since JD2443000 - see Table.
W     Tau    <P> value is given in the Table.
             P var. Max = 2415320 + 274.1d*E (JD2410360 - 15500),
             Max = 2421995 + 266.1d*E (JD2415500 - 22500),
             Max = 2425135 + 260.5d*E (JD2422500 - 28800),
             Max = 2438837 + 245.4d*E (JD2428800 - 39100) [00001].
Z     Tau    VB A (B 13.6m, 4", 45deg).
             P var. Max = 2425115 + 499.90d*E (JD2415100 - 26500)
             Max = 2438768 + 486.20d*E (JD2426500 - 39000);
             since JD2439000 - see Table.
RR    Tau    Spectrum description and the photographs of the nebula
             [04002].
RU    Tau    VB A (B 4"). P var. Max = 2426004 + 545.3d*E
             (JD2415009 - 27500). Max = 2434309 + 604.0d*E
             (JD2427500 - 34500); since JD2437500 - see Table.
RV    Tau    OH maser. Mean brightness varies: Min = 2417553 + 1224d*E
             [00580].
RW    Tau    VB A (12.5m, 1.3", 172deg, 1959). dI = 0.020P; Min II 8.09.
             P var. Min I = 2417198.410 + 2.7688665d*E +
             0.038d*sin(0.0818deg*(E - 100)) (JD2409913 - 24150),
             Min I = 2434423.3571 + 2.7688209d*E (JD2424150 - 37000)
             [05460]; Min I = 2437164.4860 + 2.7688480d*E
             (JD2437000 - 39900) [07531]; Min I = 2442776.93772 +
             2.76884463d*E (JD2439855 - 42780) [08593]; Min I =
             2442776.9313 + 2.7688396d*E (JD2442780 - 45750)
             [09084]; since JD2445750 - see Table. The shape of the
             light curve varies.
RX    Tau    OH, H2O maser. P var. Max = 2423561 + 338.4d*E
             (JD2417155 - 24000); Max = 2430505 + 330.2d*E
             (JD2424000 - 30700); Max = 2437963 + 339.3d*E
             (JD2430700 - 38000); since JD2438000 - see Table.
RY    Tau    SB1. The photographs of the nebula and spectrum
             description [05064]. Long period light variations are
             possible with cycles 70.25, 15.9, 9.4 and 5.84 years
             [09993].
RZ    Tau    Min II 10.66. P var. Min I = 2424032.1426 +
             0.41567109d*E (JD2424000 - 34100) [00312];
             since JD2436000 - see Table.
SS    Tau    P var [03506]. Max = 2420894.2339 + 0.3699665d*E
             (JD2420890 - 21300) [09995]; Max = 2426669.080 +
             0.3699687d*E (JD2426400 - 26700) [00320]; Max =
             2428843.856 + 0.3699231d*E (JD2426700 - 30300),
             Max = 2431392.603 + 0.369912d*E (JD2430300 - 31400),
             Max = 2432118.794 + 0.369937d*E (JD2431400 - 32150),
             Max = 2432857.884 + 0.3699146d*E (JD2432150 - 35000),
             Max = 2435055.528 + 0.3699066d*E (JD2435000 - 36400),
             Max = 2437313.503 + 0.3699266d*E (JD2436400 - 37320),
             Max = 2437960.419 + 0.369878d*E (JD2437300 - 37960),
             Max = 2437960.419 + 0.369938d*E (JD2437960 - 38740);
             since JD2438740 - see Table.
SV    Tau    Min II 9.8.
SW    Tau    P var. Max = 2432049.856 + 1.583623d*E (JD2418240 - 36000);
             since JD2436000 - see Table.
SX    Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
SY    Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
SZ    Tau    The member of the halo of the open cluster NGC 1647.
             P var. Max = 2410000.60 + 3.1487d*E (JD2412000 - 20200)
             [09996]; Max = 2419267.519 + 3.149046d*E
             (JD2419260 - 34650); since JD2434650 - see Table.
TT    Tau    P = 364d? [00589].
TY    Tau    In the region of the hyades cluster. Not a member of
             the cluster. According to [09997], Min = 2422291.303 +
             0.539250d*E.
UU    Tau    In the region of the Pleiades cluster. Not a member of
             the cluster.
UX    Tau    VB A (B 13.67m V, M2.5 VE, 5.74", 270.1deg, 1944).
UZ    Tau    VB A (B 15.16m B, M4VE (Li), 3.7", 271.5deg, 1944).
             The range of the combined light variation is given in the
             Table.
VW    Tau    The chart in [06286] is wrong.
WW    Tau    P var. P = 114.8d (JD2414800 - 20800). P = 124.4d
             (JD2420800 - 23700) [00634]; P = 114d (JD2424800 - 26300),
             P = 139d (JD2426300 - 27700) [00310]; P = 114d
             (JD2427900 - 30800), P = 131d (JD2430800 - 31500),
             P = 109d (JD2431500 - 33400) [00364]; since
             JD2433400 - see Table.
WY    Tau    Min II 11.73. P var? [10048].
WZ    Tau    VB.
XZ    Tau    VB A (B = HL Tau, 23", 273deg).
YZ    Tau    [Fe/H] = -1.53. In the region of the Pleiades cluster.
             Not a member of the cluster.
             There is a square term in the elements: -6d*10**(-11)*E**2.
AA    Tau    Cyclic light variation with P = 4.5d and 2d [10003] and
             also 8.2d [10004] is possible.
AC    Tau    d = 0.025P. P var?
AH    Tau    Min II 11.85. P var? In the region of the Pleiades
             cluster. Not a member of the cluster.
AL    Tau    P var. The depth of Min II 0.15m.
AM    Tau    d = 0.012P:. P var. Min I = 2427534.444 + 2.044018d*E
             (JD2425580 - 27540), Min I = 2435019.436 +
             2.043935d*E (JD2433320 - 37020); since JD2442365 - see
             Table.
AN    Tau    Min II 10.5; Min II - Min I = 0.53P. P var.
AP    Tau    Min II 14.7; Min II - Min I = 0.48P.
AS    Tau    P var. Min I = 2439390.595 + 3.4835542d*E
             (JD2419440 - 44300) [07806]; since JD2444300 - see Table.
AU    Tau    P var. Max = 2426642 + 71.0d*E (JD2426290 - 30400)
             [00310]; since JD2438000 - see Table.
AW    Tau    OH, H2O maser. P var. Max = 2426278 + 690d*E
             (JD2416100 - 33850) [00609]; since JD2433850 - see Table.
BB    Tau    SC 7/7 e.
BK    Tau    In the region of the Pleiades cluster. Not a member of
             the cluster.
BN    Tau    P var. Min I = 2435460.370 + 4.2542044d*E
             (JD2419000-39100) [05466]; since JD2443000 - see Table.
BP    Tau    There are quasisinusoidal light variations with P = 7.6d
             [10011].
BU    Tau    Pleione. The member of the Pleiades cluster.
BV    Tau    Min II 11.9.
BW    Tau    3C 120. Seyfert galaxy; Z = 0.033. Spectrum description
             [10012].
CD    Tau    VB A (B 9.88m, 9.9", 148.8deg). Min II 7.31.
             In the region of the open cluster CR 65.
CF    Tau    d = 0.02P; Min II 10.2;
CH    Tau    The epoch of Min brightness is given.
CM    Tau    SN 1054 in the Crab nebula (NGC 1952 = M1); pulsar NP 0532.
             The outburst epoch is JD2106210:. The pulsed radiation
             varies precisely in phase over the whole spectrum, from
             radio waves to gamma rays with P = 0.033S in the range
             13.9m - 17.7m V. P var [10017, 10018]: 0.033095563927s
             (JD2440297.5094) <= P <= 0.033242051159s (JD2444312.750).
CR    Tau    P = 1.362692d?
CT    Tau    Min II 11.12. P var. Min I = 2437312.369 + 0.6668274d*E
             (JD2432700 - 38790) [10010]; since JD2441400 - see Table.
CU    Tau    In the region of the Pleiades cluster. Not a member of
             the cluster. Min II 11.90. P var. Min I =
             2431822.5193 + 0.4126022d*E (JD2431060 - 2890)
             [00604]; since JD2440960 - see Table.
CZ    Tau    VB B (A = DD Tau; B 31", 13deg).
DD    Tau    VB A (B = CZ Tau; 31", 13deg.
DE    Tau    VB A (B 26", 10deg).
DG    Tau    Connected with a small bright arc-shaped nebula.
DH    Tau    VB A (B = DI Tau, 16", 125deg). According to [10004] there
             is periodical light variability with P = 7.0d and
             A = 0.4m V.
DI    Tau    VB B (A = DH Tau; B 16", 125deg).
             According to [10004] there is
             periodical light variability with P ~7.0d and A < 0.4m V.
DL    Tau    VB A (B 17m V, 12", 333deg).
             Cyclic light variation with P = 2.7d is present [10003].
DN    Tau    There are sinusoidal light variations with
             P = 6.6d [10011].
DO    Tau    Connected with a small bright arc-shaped nebula.
DS    Tau    VB A (B 13.7m, 4", 288deg). Range of Combined light
             variation of the pair is given in the Table.
EI    Tau    VB?
EQ    Tau    Min II 10.97. In the region of the Pleiades cluster.
             Not a member of the cluster.
ES    Tau    Min II 14.4; Min II - Min I = 0.52P; d = 0.005P.
ET    Tau    Min II 9.3.
EY    Tau    The member of the Hyades cluster.
EZ    Tau    The member of the Hyades cluster.
FH    Tau    The member of the Hyades cluster.
FL    Tau    The member of the Pleiades cluster.
FS    Tau    VB A (B 16", 289deg).
FV    Tau    VB A (B 13", 103deg).
FW    Tau    VB A (B 13", 243deg).
FY    Tau    VB B (A = FZ Tau, B 17", 250deg.)
FZ    Tau    VB A (B = FY Tau, 17", 250deg).
GG    Tau    VB A (B 18.5m, 12", 205deg).
GH    Tau    VB B (A = V807 Tau; B 21.4", 193deg).
GI    Tau    VB B (A = GK Tau; B 13", 329deg). There are
             quasisinusoidal light variations with P = 7.2d [10011].
             Connected with a small bright arc-shaped nebula.
GK    Tau    VB A (B = GI Tau, 13", 329deg).
             There are quasisinusoidal light variations with P = 4.6d
             [10011]. Connected with a small bright arc-shaped nebula.
GL    Tau    The central star of the planetary nebula PK 174 -14deg 1.
GP    Tau    P2 = 1000d.
GR    Tau    dI = 0.068P; Min II 10.49; Mim II - Min I = 0.516P.
GS    Tau    SB1 (Porb = 7.227424d [06568]). The epoch of Min
             brightness is given.
GU    Tau    VB A (B 11", 299deg).
GV    Tau    Herbig-haro object.
GW    Tau    Min II 11.7. P var?
GX    Tau    VB A (B 11", 310deg).
HK    Tau    VB A (B 21m, 2", 180deg).
HL    Tau    VB B (A = XZ Tau; B 23", 273deg). Connected with a
             small bright arc-shaped nebula.
HN    Tau    VB A (B 18m, 3.3", 205deg).
HO    Tau    VB A (B 8", 110deg).
HP    Tau    Connected with a small bright arc-shaped nebula.
             According to [10004] there is periodical variability
             with P = 1.2d.
HR    Tau    VB B (A = HS Tau; B 14", 119deg).
HS    Tau    VB A (B = HR Tau; 14", 119deg).
HU    Tau    Min II 5.91.
HW    Tau    Minor planet (49) Pales.
HZ    Tau    In the region of the Pleiades cluster. Possible
             member of the cluster.
II    Tau    In the region of the Pleiades cluster.
             Possible member of the hyades cluster
IK    Tau    OH, H2O, SiO maser.
IM    Tau    P var. Max = 2439792.398 + 0.144969d*E (JD2439790 -
             43130) [10019]; P1 = 0.109016d, P1/P0 = 0.752.
             Since JD2444230 - see Table.
IN    Tau    mu = 0.121", P = 105deg. The member of the Hyades cluster?
IO    Tau    In the region of the Hyades cluster.
IQ    Tau    VB A (B 17m, 11", 298deg).
IS    Tau    SVS 1319 [04051].
             The star N23 with Halpha emission [00596]. In the map given
             in [00596] erroneously designated as N26 in contradiction
             with the co-ordinates given in the same paper. It was the
             reason for different mistakes when the
             star was identified by some other investigators.
IT    Tau    SVS 1320 [04051].
             The star N26 with Halpha emission [00596].
             In the map given in [00596] IS Tau erroneously designated
             as N26 in contradiction with the co-ordinates given in the
             same paper. It was the reason for different mistakes when
             IS Tau was identified by some other investigators.
KK    Tau    In the region of the Pleiades cluster.
KL    Tau    In the region of the Pleiades cluster.
KM    Tau    In the region of the Pleiades cluster.
KN    Tau    In the region of the Pleiades cluster.
KO    Tau    In the region of the Pleiades cluster.
KP    Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
KQ    Tau    In the region of the Pleiades cluster.
KR    Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
KS    Tau    In the region of the Pleiades cluster.
KT    Tau    In the region of the Pleiades cluster.
KU    Tau    In the region of the Pleiades cluster.
KV    Tau    In the region of the Pleiades cluster.
KW    Tau    In the region of the Pleiades cluster.
KX    Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
KY    Tau    The member of the Pleiades cluster.
KZ    Tau    In the region of the Pleiades cluster.
LL    Tau    In the region of the Pleiades cluster.
LM    Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
LN    Tau    In the region of the Pleiades cluster.
LO    Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
LP    Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
LQ    Tau    In the region of the Pleiades cluster.
LR    Tau    In the region of the Pleiades cluster. Possible member
             of the Hyades cluster.
LS    Tau    In the region of the Pleiades cluster.
LT    Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
LU    Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
LV    Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
LW    Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
LX    Tau    In the region of the Pleiades cluster.
LY    Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
LZ    Tau    The member of the Pleiades cluster.
MM    Tau    The member of the Pleiades cluster.
MN    Tau    In the region of the Pleiades cluster.
MO    Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
MP    Tau    In the region of the Pleiades cluster.
MQ    Tau    In the region of the Pleiades cluster.
MR    Tau    The member of the Pleiades cluster.
MS    Tau    The member of the Pleiades cluster.
MT    Tau    In the region of the Pleiades cluster. Not a member
             of the  cluster.
MU    Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
MV    Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
MW    Tau    In the region of the Pleiades cluster.
MX    Tau    The member of the Pleiades cluster.
MY    Tau    The member of the Pleiades cluster.
MZ    Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
NN    Tau    In the region of the Pleiades cluster.
NO    Tau    In the region of the Pleiades cluster.
NP    Tau    The member of the Pleiades cluster.
NQ    Tau    In the region of the Pleiades cluster.
NR    Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
NS    Tau    In the region of the Pleiades cluster.
NT    Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
NU    Tau    In the region of the Pleiades cluster.
NV    Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
NW    Tau    In the region of the Pleiades cluster.
NX    Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
NY    Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
NZ    Tau    In the region of the Pleiades cluster.
OO    Tau    In the region of the Pleiades cluster.
OP    Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
OQ    Tau    In the region of the Pleiades cluster.
OR    Tau    The member of the Pleiades cluster.
OS    Tau    The member of the Pleiades cluster.
OT    Tau    The member of the Pleiades cluster.
OU    Tau    Max = 2444896.758 + 0.39701d*E, M - m = 0.5P, A(V) =
             0.13m [10052].
             The member of the Pleiades cluster.
OW    Tau    The member of the Pleiades cluster.
OX    Tau    In the region of the Pleiades cluster.
OY    Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
OZ    Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
PP    Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
PQ    Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
PR    Tau    The member of the Pleiades cluster.
PS    Tau    In the region of the Pleiades cluster.
PT    Tau    The member of the Pleiades cluster.
PU    Tau    In the region of the Pleiades cluster.
PV    Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
PW    Tau    In the region of the Pleiades cluster.
PZ    Tau    In the region of the Pleiades cluster.
QQ    Tau    SB2. The member of the Pleiades cluster.
QR    Tau    In the region of the Pleiades cluster.
QS    Tau    In the region of the Pleiades cluster.
QT    Tau    In the region of the Pleiades cluster.
QU    Tau    VB A (B 18.0m, 4.0", 135deg). In the region of the
             Pleiades cluster.
QV    Tau    In the region of the Pleiades cluster.
QW    Tau    In the region of the Pleiades cluster.
QX    Tau    The member of the Pleiades cluster.
             Max = 2444896.79 + 0.483d*E, M - m = 0.5P, A(V) = 0.125m
             [10052].
QY    Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
QZ    Tau    In the region of the Pleiades cluster.
V0335 Tau    In the region of the Pleiades cluster.
V0336 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0337 Tau    In the region of the Pleiades cluster.
V0338 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0339 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0340 Tau    In the region of the Pleiades cluster.
V0341 Tau    In the region of the Pleiades cluster.
V0342 Tau    In the region of the Pleiades cluster.
V0343 Tau    The member of the Pleiades cluster.
V0344 Tau    In the region of the Pleiades cluster.
V0345 Tau    In the region of the Pleiades cluster.
V0346 Tau    The member of the Pleiades cluster.
V0347 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0348 Tau    In the region of the Pleiades cluster.
V0349 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0350 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0351 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0352 Tau    In the region of the Pleiades cluster.
V0353 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0354 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0355 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0356 Tau    In the region of the Pleiades cluster.
V0357 Tau    The member of the Pleiades cluster.
V0358 Tau    The member of the Pleiades cluster.
V0359 Tau    In the region of the Pleiades cluster.
V0360 Tau    In the region of the Pleiades cluster.
V0361 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0362 Tau    In the region of the Pleiades cluster.
V0363 Tau    In the region of the Pleiades cluster. Possible member
V0364 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0365 Tau    In the region of the Pleiades cluster.
V0366 Tau    The member of the Pleiades cluster.
V0367 Tau    In the region of the Pleiades cluster.
V0368 Tau    In the region of the Pleiades cluster.
V0369 Tau    In the region of the Pleiades cluster.
V0370 Tau    The member of the Pleiades cluster.
V0371 Tau    VB (Delta(m) ~1m, 1.5"). The member of the Pleiades
             cluster.
V0372 Tau    The member of the Pleiades cluster.
V0373 Tau    In the region of the Pleiades cluster.
V0374 Tau    In the region of the Pleiades cluster.
V0375 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0376 Tau    The member of the Pleiades cluster.
V0377 Tau    The member of the Pleiades cluster.
V0378 Tau    The member of the Pleiades cluster.
V0379 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0380 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0381 Tau    The member of the Pleiades cluster.
V0382 Tau    The member of the Pleiades cluster.
V0383 Tau    In the region of the Pleiades cluster.
V0384 Tau    The member of the Pleiades cluster.
V0385 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0386 Tau    TCSN 437. In the region of the Pleiades cluster.
V0387 Tau    In the region of the Pleiades cluster.
V0388 Tau    In the region of the Pleiades cluster.
V0389 Tau    TCSN 439. In the region of the Pleiades cluster.
V0390 Tau    In the region of the Pleiades cluster.
V0392 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0394 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0395 Tau    In the region of the Pleiades cluster.
V0396 Tau    In the region of the Pleiades cluster.
V0397 Tau    In the region of the Pleiades cluster.
V0398 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0399 Tau    The member of the Pleiades cluster.
V0400 Tau    In the region of the Pleiades cluster.
V0401 Tau    In the region of the Pleiades cluster.
V0402 Tau    The member of the Pleiades cluster.
V0403 Tau    The member of the Pleiades cluster.
V0404 Tau    In the region of the Pleiades cluster.
V0405 Tau    In the region of the Pleiades cluster.
V0410 Tau    There are periodical light variations with P = 1.92d,
             A(V) = 0.21m, M - m = 0.5P [10056].
V0411 Tau    mu = 0.13", P = 143deg.
             Eruptive white dwarf. Usually there are quasi-perio-
             dic variations with A ~0.3m and periods P0 = 12.436
             Min and P1 = 8.237 Min (P1/P0 = 0.6624) which are
             nonlinearly modulated by the third period PL ~0.135d
             (probably by the orbital period of a faint companion).
V0421 Tau    Minor planet (586) Thekla.
V0423 Tau    Min II 15.8.
V0425 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0426 Tau    In the region of the Pleiades cluster.
V0427 Tau    In the region of the Pleiades cluster.
V0428 Tau    In the region of the Pleiades cluster.
V0429 Tau    In the region of the Pleiades cluster.
V0430 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0431 Tau    In the region of the Pleiades cluster.
V0432 Tau    In the region of the Pleiades cluster.
V0433 Tau    In the region of the Pleiades cluster.
V0434 Tau    In the region of the Pleiades cluster.
V0435 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0436 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0437 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0438 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0439 Tau    In the region of the Pleiades cluster.
V0440 Tau    In the region of the Pleiades cluster.
V0441 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0442 Tau    In the region of the Pleiades cluster.
V0443 Tau    In the region of the Pleiades cluster.
V0444 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0445 Tau    In the region of the Pleiades cluster.
V0446 Tau    The member of the Pleiades cluster.
V0447 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0448 Tau    The member of the Pleiades cluster.
V0449 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0451 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0452 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0453 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0454 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0455 Tau    In the region of the Pleiades cluster.
V0456 Tau    In the region of the Pleiades cluster.
V0457 Tau    In the region of the Pleiades cluster.
V0458 Tau    In the region of the Pleiades cluster.
V0459 Tau    In the region of the Pleiades cluster.
V0460 Tau    In the region of the Pleiades cluster.
V0461 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0462 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0463 Tau    In the region of the Pleiades cluster.
V0464 Tau    In the region of the Pleiades cluster.
V0465 Tau    In the region of the Pleiades cluster.
V0466 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0467 Tau    In the region of the Pleiades cluster.
V0468 Tau    In the region of the Pleiades cluster.
V0469 Tau    In the region of the Pleiades cluster.
V0470 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0471 Tau    The member of the Hyades cluster. mu alpha =  + 0.117",
             mu delta = -0.020".
             EA/D/(RS + WD) + XP. d = 0.0625P.
             There occurs a total eclipse of the white dwarf in
             Min I (A = 0.04m V, 0.36m U).
             P var. Min I = 2440612.67083 + 0.52118321d*E
             (JD2440570 - 970) [06250]; Min I = 2440898.80038 +
             0.52118376d*E (JD2440880 - 41360), Min I =
             2441665.46153 + 0.52118329d*E (JD2441660 -
             42100) [10058]; since JD2441900 - see Table.
             Wave-like distorsion with the amplitude from 0.05m
             up to 0.27m and with the period close to the orbital
             one is observed in the light curve outside eclipses;
             sometimes there are also flares. The wave is migrating on
             phase in the direction of phase decreasing
             with a migration period of 191d [10060] or ~250d
             [10061]. The period of white dwarf rotation derived
             through X-ray observations Ppuls = 554.73s [10062].
V0472 Tau    In the region of the Pleiades cluster.
V0473 Tau    P = 2.7800d?
V0474 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0475 Tau    In the region of the Pleiades cluster.
V0476 Tau    In the region of the Pleiades cluster.
V0477 Tau    In the region of the Pleiades cluster.
V0478 Tau    In the region of the Pleiades cluster.
V0479 Tau    VB A (BC 8.90m, 59", 357deg); (k - b)2 = 0.40.
V0480 Tau    VB A (B 10.4m, 176", 303deg). The member of the Hyades
             cluster.
V0481 Tau    In the region of the Pleiades cluster.
V0483 Tau    The member of the Hyades cluster.
V0484 Tau    The member of the Hyades cluster.
V0485 Tau    In the region of the Pleiades cluster.
V0486 Tau    Epoch of Max (U) is given.
             P =/ 10.61d? [10063].
V0487 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
             On the photograph west is at the top and
             south to the right.
V0488 Tau    The member of the Pleiades cluster.
V0489 Tau    In the region of the Pleiades cluster.
V0490 Tau    In the region of the Pleiades cluster.
V0491 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0492 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0493 Tau    In the region of the Pleiades cluster.
V0494 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0495 Tau    In the region of the Pleiades cluster.
V0496 Tau    In the region of the Pleiades cluster.
V0497 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0498 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0499 Tau    In the region of the Pleiades cluster.
V0500 Tau    The member of the Pleiades cluster.
V0501 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0502 Tau    The member of the Pleiades cluster.
V0503 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0504 Tau    In the region of the Pleiades cluster.
V0506 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0507 Tau    In the region of the Pleiades cluster.
V0508 Tau    In the region of the Pleiades cluster.
V0509 Tau    In the region of the Pleiades cluster.
V0510 Tau    In the region of the Pleiades cluster.
V0511 Tau    In the region of the Pleiades cluster.
V0512 Tau    In the region of the Pleiades cluster.
V0513 Tau    In the region of the Pleiades cluster.
V0514 Tau    In the region of the Pleiades cluster.
V0515 Tau    In the region of the Pleiades cluster.
V0516 Tau    In the region of the Pleiades cluster.
V0517 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0518 Tau    VB B (A 14.4m; B 10", 80deg). The member of the
             Pleiades cluster.
V0519 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0520 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0521 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0522 Tau    In the region of the Pleiades cluster.
V0523 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0524 Tau    In the region of the Pleiades cluster.
V0525 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0526 Tau    In the region of the Pleiades cluster.
V0527 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0528 Tau    In the region of the Pleiades cluster.
V0529 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0530 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0531 Tau    In the region of the Pleiades cluster.
V0532 Tau    In the region of the Pleiades cluster.
V0533 Tau    In the region of the Pleiades cluster.
V0534 Tau    In the region of the Pleiades cluster.
V0535 Tau    In the region of the Pleiades cluster.
V0536 Tau    In the region of the Pleiades cluster.
V0537 Tau    In the region of the Pleiades cluster.
V0538 Tau    The member of the Pleiadea cluster.
V0539 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0540 Tau    The member of the Pleiades cluster.
V0541 Tau    The member of the Pleiades cluster.
V0542 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0543 Tau    In the region of the Pleiades cluster.
V0544 Tau    In the region of the Pleiades cluster.
V0545 Tau    Max = 2444896.678 + 0.355d*E, M - m = 0.42P, A(V) =
             0.09m [10052]. The member of the Pleiades cluster.
V0546 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0547 Tau    In the region of the Pleiades cluster.
V0548 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0549 Tau    In the region of the Pleiades cluster.
V0550 Tau    The member of the Pleiades cluster.
V0551 Tau    In the region of the Pleiades cluster.
V0552 Tau    In the region of the Pleiades cluster.
V0553 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0554 Tau    In the region of the Pleiades cluster.
V0555 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0556 Tau    In the region of the Pleiades cluster.
V0557 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0558 Tau    In the region of the Pleiades cluster.
V0559 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0560 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0561 Tau    In the region of the Pleiades cluster.
V0562 Tau    In the region of the Pleiades cluster.
V0563 Tau    In the region of the Pleiades cluster.
V0564 Tau    In the region of the Pleiades cluster.
V0565 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0566 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0567 Tau    In the region of the Pleiades cluster.
V0568 Tau    In the region of the Pleiades cluster.
V0569 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0570 Tau    In the region of the Pleiades cluster.
V0571 Tau    In the region of the Pleiades cluster.
V0572 Tau    In the region of the Pleiades cluster.
V0573 Tau    In the region of the Pleiades cluster.
V0574 Tau    In the region of the Pleiades cluster.
V0575 Tau    In the region of the Pleiades cluster.
V0576 Tau    In the region of the Pleiades cluster.
V0577 Tau    In the region of the Pleiades cluster.
V0578 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0579 Tau    In the region of the Pleiades cluster.
V0581 Tau    In the region of the Pleiades cluster.
V0582 Tau    In the region of the Pleiades cluster.
V0583 Tau    In the region of the Pleiades cluster.
V0584 Tau    In the region of the Pleiades cluster.
V0585 Tau    In the region of the Hyades cluster.
V0589 Tau    In the region of the Hyades cluster.
V0594 Tau    In the region of the Pleiades cluster.
V0595 Tau    In the region of the Pleiades cluster.
V0596 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0597 Tau    In the region of the Pleiades cluster.
V0598 Tau    In the region of the Pleiades cluster.
V0599 Tau    In the region of the Pleiades cluster.
V0600 Tau    In the region of the Pleiades cluster.
V0601 Tau    In the region of the Pleiades cluster.
V0602 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0603 Tau    In the region of the Pleiades cluster.
V0604 Tau    In the region of the Pleiades cluster.
V0605 Tau    In the region of the Pleiades cluster.
V0606 Tau    In the region of the Pleiades cluster.
V0607 Tau    In the region of the Pleiades cluster.
V0608 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0609 Tau    In the region of the Pleiades cluster.
V0610 Tau    The member of the Pleiades cluster.
V0611 Tau    In the region of the Pleiades cluster.
V0612 Tau    In the region of the Pleiades cluster.
V0613 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0614 Tau    In the region of the Pleiades cluster.
V0615 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0617 Tau    In the region of the Pleiades cluster.
V0618 Tau    In the region of the Pleiades cluster.
V0619 Tau    In the region of the Pleiades cluster.
V0620 Tau    In the region of the Pleiades cluster.
V0621 Tau    In the region of the Pleiades cluster.
V0622 Tau    In the region of the Pleiades cluster.
V0623 Tau    The member of the Pleiades cluster.
V0624 Tau    The value of P1(A1 = 0.01m) is given in the Table.
             P2 = 0.017d, A2 = 0.007m. The member of the Pleiades
             cluster.
V0625 Tau    In the region of the Pleiades cluster.
V0626 Tau    In the region of the Pleiades cluster.
V0627 Tau    The member of the Pleiades cluster.
V0629 Tau    In the region of the Pleiades cluster.
V0630 Tau    In the region of the Pleiades cluster.
V0631 Tau    The member of the Pleiades cluster.
V0632 Tau    The member of the Pleiades cluster.
V0633 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0634 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0635 Tau    The member of the Pleiades cluster.
V0636 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0637 Tau    In the region of the Pleiades cluster.
V0638 Tau    The member of the Pleiades cluster.
V0639 Tau    In the region of the Pleiades cluster.
V0640 Tau    In the region of the Pleiades cluster.
V0641 Tau    Max = 2444896.744 + 1.22d*E; M - m = 0.5P, A(V) = 0.03m
             [10052]. The member of the Pleiades cluster.
V0642 Tau    The member of the Pleiades cluster.
V0643 Tau    The member of the Pleiades cluster.
V0644 Tau    The member of the Pleiades cluster.
V0645 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0646 Tau    The member of the Pleiades cluster.
V0647 Tau    The value
             of P1(A1 = 0.011m) is given in the Table.
             P2 = 0.070d, A2 = 0.006m. The member of the Pleiades
             cluster.
V0648 Tau    In the region of the Pleiades cluster.
V0649 Tau    In the region of the Pleiades cluster.
V0650 Tau    The member of the Pleiades cluster.
V0651 Tau    In the region of the Pleiades cluster.
V0652 Tau    The member of the Pleiades cluster.
V0653 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0654 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0655 Tau    In the region of the Pleiades cluster.
V0656 Tau    In the region of the Pleiades cluster.
V0657 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0658 Tau    In the region of the Pleiades cluster.
V0659 Tau    In the region of the Pleiades cluster.
V0660 Tau    Max = 2444896.453 + 0.23541d*E, M - m = 0.5P, A(V) =
             0.20m [10052]. The member of the Pleiades cluster.
V0661 Tau    In the region of the Pleiades cluster.
V0662 Tau    In the region of the Pleiades cluster.
V0663 Tau    In the region of the Pleiades cluster.
V0664 Tau    The member of the Pleiades cluster.
V0665 Tau    In the region of the Pleiades cluster. Not a member
             of the region.
V0666 Tau    In the region of the Pleiades cluster.
V0667 Tau    The member of the Pleiades cluster.
V0668 Tau    In the region of the Pleiades cluster.
V0669 Tau    In the region of the Pleiades cluster.
V0670 Tau    In the region of the Pleiades cluster.
V0671 Tau    In the region of the Pleiades cluster.
V0672 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0673 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0674 Tau    In the region of the Pleiades cluster.
V0675 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0676 Tau    In the region of the Pleiades cluster.
V0677 Tau    The member of the Pleiades cluster.
V0678 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0679 Tau    The member of the Pleiades cluster.
V0680 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0681 Tau    In the region of the Pleiades cluster.
V0682 Tau    In the region of the Pleiades cluster.
V0683 Tau    In the region of the Pleiades cluster.
V0684 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0685 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0686 Tau    In the region of the Pleiades cluster.
V0687 Tau    In the region of the Pleiades cluster.
V0688 Tau    In the region of the Pleiades cluster.
V0689 Tau    In the region of the Pleiades cluster.
V0690 Tau    In the region of the Pleiades cluster.
V0691 Tau    In the region of the Pleiades cluster.
V0692 Tau    In the region of the Pleiades cluster. Possible member
             of the cluster.
V0693 Tau    In the region of the Pleiades cluster.
V0694 Tau    In the region of the Pleiades cluster.
V0696 Tau    The member of the Hyades cluster.
V0697 Tau    The member of the Hyades cluster.
V0698 Tau    Type INB?
V0700 Tau    The member of the Pleiades cluster.
V0701 Tau    In the region of the Pleiades cluster.
V0702 Tau    In the region of the Pleiades cluster.
V0703 Tau    The member of the Pleiades cluster.
V0705 Tau    In the region of the Pleiades cluster.
V0706 Tau    In the region of the Pleiades cluster.
V0707 Tau    In the region of the Pleiades cluster.
V0709 Tau    In the region of the Pleiades cluster.
V0710 Tau    VB A (B 16m, 3.5", 180deg).
V0711 Tau    VB A (B 8.83m, A = 8.023", E = 0.18, Porb = 2101 yr);
             SB2 (Porb = 2.83774d [10070]).
             Migration period of the distortion wave is about
             10.5 yr [10072].
             The range of combined light variation is given.
V0712 Tau    In the region of the Pleiades cluster.
V0713 Tau    In the region of the Pleiades cluster.
V0714 Tau    In the region of the Pleiades cluster.
V0715 Tau    In the region of the Pleiades cluster.
V0716 Tau    In the region of the Pleiades cluster.
V0717 Tau    In the region of the Pleiades cluster.
V0718 Tau    In the region of the Hyades cluster.
V0725 Tau    SB1 (Porb = 110.8d [10076]).
             X-ray outbursts occur periodically near
             the periastron passages of the pulsar with P = Porb.
             The amplitude of the corresponding variations of
             visual brightness of the system A(V) = 0.03m. The period
             of pulsar rotation Prot var [10077].
             Prot = 104.17s (JD2442531), 103.806s (JD2442728),
             103.882s (JD2443505), 103.8402s (JD2443620)
             [10074]; 103.647s (JD2444521), 103.423s
             (JD2445292), 103.3429ss(JD2445623) [10078].
V0726 Tau    Min II 11.2.
V0727 Tau    In the region of the Pleiades cluster.
V0728 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0729 Tau    Max = 2439024.46 + 152.35d*E (JD2438680 - 39415);
             Max = 2440127.78 + 313.86d*E (JD2439415 - 40510).
             H2O maser.
V0732 Tau    In the region of the Pleiades cluster.
V0733 Tau    In the region of the Pleiades cluster.
V0734 Tau    In the region of the Pleiades cluster.
V0735 Tau    In the region of the Pleiades cluster.
V0736 Tau    In the region of the Pleiades cluster.
V0737 Tau    In the region of the Pleiades cluster.
V0738 Tau    In the region of the Pleiades cluster. The chart in [08559]
             is wrong.
V0739 Tau    In the region of the Pleiades cluster.
V0740 Tau    In the region of the Pleiades cluster.
V0741 Tau    In the region of the Pleiades cluster.
V0742 Tau    In the region of the Pleiades cluster.
V0743 Tau    In the region of the Pleiades cluster.
V0744 Tau    In the region of the Pleiades cluster.
V0746 Tau    In the region of the Pleiades cluster.
V0747 Tau    In the region of the Pleiades cluster.
V0748 Tau    In the region of the Pleiades cluster.
V0749 Tau    In the region of the Pleiades cluster.
V0750 Tau    In the region of the Pleiades cluster.
V0751 Tau    In the region of the Pleiades cluster.
V0752 Tau    In the region of the Pleiades cluster.
V0753 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0754 Tau    In the region of the Pleiades cluster.
V0755 Tau    In the region of the Pleiades cluster.
V0756 Tau    In the region of the Pleiades cluster.
V0757 Tau    In the region of the Pleiades cluster.
V0758 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0759 Tau    In the region of the Pleiades cluster.
V0760 Tau    In the region of the Pleiades cluster.
V0761 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0762 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0763 Tau    In the region of the Pleiades cluster.
V0764 Tau    In the region of the Pleiades cluster.
V0765 Tau    In the region of the Pleiades cluster.
V0767 Tau    In the region of the Pleiades cluster.
V0768 Tau    In the region of the Pleiades cluster.
V0769 Tau    In the region of the Pleiades cluster.
V0770 Tau    In the region of the Pleiades cluster.
V0771 Tau    In the region of the Pleiades cluster.
V0772 Tau    In the region of the Pleiades cluster.
V0773 Tau    There are also quasisinusoidal light variations with
             P = 3.43d and A(V) = 0.13m [10056].
V0774 Tau    VB A (B 6.96m, G5IV, 66.8", 315deg).
V0775 Tau    The member of the Hyades cluster.
V0776 Tau    VB A (B 7.5m, 1.4", 333deg, 1958; C 8.7m, 77.2", 233deg,
             1925); SB1 (Porb = 57.25d). The member of the
             Hyades cluster.
V0777 Tau    VB A (B 8.12m V, 0.0088", 173.2deg, 1980.6).
             The member of the Hyades cluster.
V0778 Tau    Min II 17.0. P var. Min I = 2438680.546 + 0.434842d*E
             (JD2436528 - 38841); Min I = 2439765.488 + 0.434846d*E
             (JD2439559 - 41031); since JD2440129 - see Table.
V0780 Tau    VB A (B 15.8m V, 0.3", 310deg, 1974); mu = 0.364",
             P = 163deg.
V0781 Tau    Min II 9.3.
V0782 Tau    In the region of the Pleiades cluster.
V0783 Tau    In the region of the Pleiades cluster.
V0784 Tau    In the region of the Pleiades cluster.
V0785 Tau    The member of the Pleiades cluster.
V0787 Tau    In the region of the Pleiades cluster.
V0788 Tau    In the region of the Pleiades cluster.
V0789 Tau    The member of the Pleiades cluster.
V0790 Tau    The member of the Pleiades cluster.
V0791 Tau    In the region of the Pleiades cluster.
V0792 Tau    Near V752 Tau. Identical to it?
             In the region of the Pleiades cluster.
V0793 Tau    The member of the Pleiades cluster.
V0794 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0795 Tau    In the region of the Pleiades cluster.
V0796 Tau    The member of the Pleiades cluster.
V0797 Tau    In the region of the Pleiades cluster. Not a member
             of the cluster.
V0798 Tau    In the region of the Pleiades cluster.
V0799 Tau    In the region of the Pleiades cluster.
V0800 Tau    In the region of the Pleiades cluster.
V0801 Tau    In the region of the Pleiades cluster.
V0802 Tau    In the region of the Pleiades cluster.
V0804 Tau    In the region of the Pleiades cluster.
V0805 Tau    The member of the Hyades cluster.
V0807 Tau    VB A (B = GH Tau, 21.4", 193deg).
V0808 Tau    Porb = 11.93d. The member of the Hyades cluster.
V1144 Tau    SB, Porb = 13.88d.
V1148 Tau    Type LBV: is also possible. SB, Porb = 2.2075d.
V1152 Tau    Type E: with P = 11.080d is also possible.
V1161 Tau    Variability needs confirmation.
V1212 Tau    Dwarf nova in Taurus.
alf   Tau    VB A (B 13.5m, M2V, 31", 110deg).
             The star is surrounded by an infrared emission envelope
             with the diameter of about 10". In the region of the
             Hyades cluster.
zet   Tau    Min II 3.05.
tet 2 Tau    VB A (B 4.85m, 0.02077", 19.6deg, 1980.59); SB1 (Porb =
             140.728D, E = 0.75 [10087]). The value of P1(A1 = 0.017m B)
             is given in the Table. P1 var. Later P1 = 0.07541d
             (A1 = 0.023m B), P2 = 0.0831d (A2 = 0.013m B). Possibly
             eclipsing with the elements:
             Min = 2445358.38 + 140.734d*E, A = 0.02m B.
             The member of the Hyades cluster.
lam   Tau    Min II 3.54. Triple system. The eclipsing system rotates
             around the third component with P = 33.025d [10090].
             In the region of the Hyades cluster.
rho   Tau    The member of the Hyades cluster.
ups   Tau    VB A (B 6.5m, 0.020"). The member of the Hyades cluster.
U     Tel    P var. Before JD2421000 Max = 2420992 + 439.13d*E [00001];
             since JD2423000 - see Table.
RR    Tel    During 1889 - 1930 12m - 14m pg (according to [00625],
             irregular variations; according to [00017],
             Max = 2411490 + 384d*E, with irregularities). During
             1930 - 1944 12.5m - 16.5m pg, Max = 2430145 + 386.73d*E
             [01649]; after 1938 an increase of mean brightness
             and of the amplitude was noted. An outburst from
             14m to 7m in October, 1944. In Max, 6.5m - 7.5m pg,
             during JD2431500 - 33000; after JD2433100 began
             to decline its mean brightness. Near the Max of the
             outburst no periodic variations was noted. During
             JD2441426 - 44899 5.06m - 6.74m J, P = 387d [09989],
             M - m = 0.5P; Min (V) = 2442551 + 374.2d*E (1961 - 1981),
             Delta(V) = 0.25m for periodic changes [10029];
             9.8m - 10.7m B, P = 395d (JD2443500 - 45500) [10030].
             In the Max of the outburst the spectrum was F5
             without emissions. During the brightness decline a
             rich emission spectrum was formed with lines of
             hydrogen, forbidden lines of metals in high stages
             of ionization, etc. Since the 1970-ies TiO absorption
             bands are being noted. Radio source, soft X-ray source.
RS    Tel    Semiregular variations, P = 45.8d [08140]. IR excess.
RV    Tel    VB (0.6", 294deg, 1946). d = 0.02P.
ST    Tel    The chart in [06286] is wrong.
SZ    Tel    Possibly identical with the star alpha = 18h 13m 16s,
             delta = -53deg 39.2', 1950.0 (RR, 15m - 16.5m pg) [10032].
             In the region of the globular cluster NGC 6584.
TT    Tel    In the region of the globular cluster NGC 6584.
TU    Tel    In the region of the globular cluster NGC 6584.
TV    Tel    In the region of the globular cluster NGC 6584.
TW    Tel    In the region of the globular cluster NGC 6584. The chart
             in [06286] is wrong.
TX    Tel    In the region of the globular cluster NGC 6584. The chart
             in [06286] is wrong.
UY    Tel    VB.
AG    Tel    nf star of a pair.
AK    Tel    Very red.
AX    Tel    [A/H] = -0.7.
BL    Tel    The depth of Min II - 0.1m pg.
             Semiregular variability of pulsational character
             (7.09m - 7.26m V) is observed outside eclipses; sometimes
             it may be represented by P = 65.1d, but sometimes (1969)
             it cannot be traced.
BO    Tel    [A/H] = -0.3.
CK    Tel    VB B (A 15.0m).
DZ    Tel    sf star of a pair.
FR    Tel    D >= 0.23P. Min II 14.0?
GH    Tel    P ~10.342d is possible.
GM    Tel    VB A.
GR    Tel    The chart in [06286] is wrong.
GY    Tel    Min II 12.0.
HH    Tel    P var slightly.
HO    Tel    Min II 8.67.
HR    Tel    EW type with twice longer P is possible.
IL    Tel    The elements need confirmation.
IQ    Tel    Min II 12.7.
KK    Tel    B - V: +0.6m: (Min light).
KN    Tel    VB A (B 16m sf).
LW    Tel    Possibly identical to NSV10695.
MT    Tel    mu alpha = -0.0127S, mu delta = -0.109".
             [Fe/H] = -1.82. Delta(S) = 9.9.
MV    Tel    EW type with twice longer P is possible.
MZ    Tel    EW type with twice longer P is possible.
NN    Tel    Min II 15.5.
NP    Tel    Min II 13.3.
NS    Tel    Min II 9.4.
NV    Tel    Min II 9.0.
OQ    Tel    sf star of a pair.
PR    Tel    Min II 11.35. Radio source PKS 1925 - 524.
             Hbeta fluctuates on ~5 min time scale.
PS    Tel    V39 (NGC 6584). Probably non-member of the cluster.
             P = 0.1422d or 0.1657d is possible.
PT    Tel    V27 (NGC 6584). Cluster non-member.
PU    Tel    V24 (NGC 6584). Cluster non-member.
PV    Tel    SB2.
PX    Tel    V15 (NGC 6584). Cluster non-member.
PZ    Tel    SB2.
QZ    Tel    The variability may be due to the fainter (B) component.
V0337 Tel    Type EW: is also possible.
R     Tri    P var. Max = 2412167 + 267.3d*E (JD2412000 - 16000);
             Max = 2416972 + 262.6d*E (JD2416000 - 20000);
             since JD2420000 - see Table. Maser (H2O).
S     Tri    P var. Max = 2418541 + 248.9d*E (JD2418000 - 31000);
             since JD2431000 - see Table.
T     Tri    P var. Max = 2420535 + 320.6d*E (JD2420000 - 27000);
             since JD2427000 - see Table.
U     Tri    Delta(S) = 1.3.
V     Tri    Min II 11.0.
X     Tri    VB A (B 13.3m, 6.7", 55.3deg, 1952). Usual brightness in
             Max 8.88. d = 0.013P; Min II 9.07. According to [10043],
             a two-peaked flare-like event of 35 min duration
             (Delta(V) = 0.33m) was observed at JD2445594.4550.
             P var. Min = 2422722.269 + 0.9715342d*E
             (JD2422700 - 26600); Min = 2426946.508 + 0.9715390d*E
             (JD2426600 - 33400); Min = 2433504.397 + 0.9715290d*E
             (JD2433400 - 35500);
             Min = 2435687.422 + 0.9715352d*E (JD2435500 - 39200);
             Min = 2439375.373 + 0.9715277d*E
             (JD2439200 - 42500) [07603]; since JD2442500 - see Table.
Y     Tri    Var No.2 (M33). VB A (B 17.28m B, 26.4" np).
RS    Tri    VB A (B 11.98m, 6.0", 214deg, 1962).
             d = 0.016P; Min II 10.4, Min II - Min I = 0.56P.
RU    Tri    VB A (B 12m, 21.8", 88deg). Min II 11.8:.
RW    Tri    The depth of Min I 1.12m - 2.21m.
             D = 0.052P - 0.086P, d ~0.03P. P var? [03434, 09858, 9859].
             Strong fluctuations of light outside eclipses. the lower
             the brightness outside the eclipse, the deeper the Min.
             In J, K light Min II of 0.16m J depth was found at the
             phase 0.50P [10053]. Flat spectrum of the accretion disc
             with emission lines.
RX    Tri    Max = 2426577 + 192d*E (JD2426500 - 31800);
             since JD2432800 - see Table. According to [04029],
             P = 100d?
RY    Tri    Red.
ST    Tri    Min II 14.5.
SW    Tri    Blazhko effect is possible.
SY    Tri    Blazhko effect is possible.
TT    Tri    In the region of the galaxy M 33.
TZ    Tri    ADS 1697 A (B 6.72m, F6V, SB2, Porb = 2.2365d,
             3.9", 71deg, 1973); SB2 (P = 14.732d). Secondary
             variations on ~100d time scale. H and K CaII emission was
             noted only for one of the two G-stars.
alf   Tri    SB (Porb = 1.767 d).
R     TrA    SB?
U     TrA    For moments of Max0 (fundamental mode) see Table.
             Max1 (first overtone) = 2443266.05 + 1.824881d*E.
RR    TrA    Min II 10.60, dII = 0.025P.
RW    TrA    (k - b)2 = 0.30. Delta(S) = 1.
SU    TrA    The chart in [06286] is wrong.
TW    TrA    VB.
TY    TrA    The chart in [06286] is wrong.
UW    TrA    The chart in [06286] is wrong.
UZ    TrA    The chart in [06286] is wrong.
XX    TrA    The chart in [06286] is wrong.
XY    TrA    The chart in [06286] is wrong.
AS    TrA    Min II 15.7.
BH    TrA    According to [04637], L type.
CI    TrA    Possibly P < 0.3d.
DI    TrA    The chart in [06286] is wrong.
DV    TrA    Three Max and three Min are observed during a cycle.
             Max1 (phi = 0.0P) 13.2m; Max2 (phi = 0.2P) 14.2m; Max3
             (phi = 0.6P) 13.5m. Min1, Min2, Min3 ~16.0m.
DZ    TrA    The chart in [06286] is wrong.
EH    TrA    Shallow Min II is possible.
EK    TrA    n star of a pair.
             For the mean cycle between normal maxima see Table. The
             mean cycle between supermaxima 442.1d (JD2435200 - 39700),
             551.5d (JD2439700 - 44050). Superhumps (delta(M) = 0.26m V)
             with P = 0.06492d, M - m = 0.26P [09945].
EL    TrA    Min II 10.9.
EM    TrA    Min II 10.4.
EN    TrA    According to [07934], RV: type.
EP    TrA    Min II 9.5.
EQ    TrA    Min II 9.0.
             P var. Min = 2416267.614 + 2.709220d*E (JD2416000 - 29000);
             since JD2429000 - see Table.
ER    TrA    P > 220d.
FH    TrA    The elements need confirmation.
FK    TrA    The elements need confirmation.
FM    TrA    P >= 220d.
GN    TrA    Min II 12.0.
HP    TrA    Deep Min II. The elements need improvement.
HV    TrA    Min II? 14.8. Min II - Min I = 0.55P.
IM    TrA    P >= 150d. Epoch of Min is given.
IW    TrA    Min II 14.5:. The elements need confirmation.
KX    TrA    2U 1639-62? P.K.326 -10deg 1. Gas velocities up to
             5000 km/s [09958].
KY    TrA    TrA X-1 = A1524-61.
KZ    TrA    4U 1626-67. Lx/Lopt ~2000. VB B (A 14.9m; B25", 189deg).
             Barycentric period parameters for pulses [04534]: Min =
             JED 2443931.2394789; P = 7.6776762s, DP/dt =
             (-4.95 +-0.02)*10**(-11). Delta(m) pulse = 0.02m - 0.17m.
             Porb = 2491.06s or 2492.32s [04558].
             Flares with Delta(m) up to 0.4m with intervals ~20 min
             correlated with X-ray flares [04536].
LM    TrA    The chart in [08661] is wrong.
LP    TrA    VB A (B 11.5m, 25", 123deg; C 12.0m, BC 6").
T     Tuc    P var. Max = 2410138 + 250.76d*E (JD2410000 - 14400);
             Max = 2414900 + 248.88d*E (JD2414400 - 22000);
             Max = 2432160 + 250.00d*E (JD2422900 - 35000);
             since JD2437700 - see Table.
U     Tuc    In the region of the Small Magellanic Cloud.
             SMS non-member.
             P var. Max = 2421190 + 258.12d*E (JD2412600 - 22000);
             Max = 2427487 + 262.83d*E (JD2422000 - 28000);
             Max = 2437808 + 257.70d*E (JD2428000 - 39150);
             since JD2440900 - see Table.
V     Tuc    In the region of the Small Magellanic Cloud.
             SMS non-member.
             The depth of Min II 0.11m.
W     Tuc    (k - b)2 = 0.09, Delta(S) = 7:. P var?
RR    Tuc    In the region of the Small Magellanic Cloud.
             VB A (B 17m, 6", 90deg).
RV    Tuc    In the region of the Small Magellanic Cloud. VB.
SS    Tuc    In the region of the Small Magellanic Cloud. HV 1877.
             Earlier was erroneously identifded with HV 1887.
SU    Tuc    In the region of the Small Magellanic Cloud. HV 1922.
             According to [09980], alternatively may be identical to
             HV 1920.
SX    Tuc    In the region of the Small Magellanic Cloud. VB (B 16m? P).
SY    Tuc    In the region of the Small Magellanic Cloud. Min II 15.4.
TV    Tuc    In the region of the Small Magellanic Cloud.
             The variable's position in 2' to the north
             of CPD -73deg 64 [09980] makes it impossible to identify
             it with HV 2041.
TZ    Tuc    In the region of the Small Magellanic Cloud.
             SMS non-member.
             VB A (B 13m sp).
UW    Tuc    In the region of the Small Magellanic Cloud.
             SMC non-member.
UX    Tuc    In the region of the Small Magellanic Cloud.
             SMS non-member.In the neighbourhood OF 47 Tuc; probably
             cluster non-member. P var. [Fe/H] = -1.8.
YY    Tuc    The elements need improvement; current elements with the
             epoch from [07984] are given.
             (k - b)2 = 0.03. Delta(S) = 8:.
AD    Tuc    In the region of the Small Magellanic Cloud.
             SMS non-member. Delta(S) = 4.9.
AF    Tuc    In the region of the Small Magellanic Cloud. SMS
             non-member.
AH    Tuc    In the region of the Small Magellanic Cloud. SMS
             non-member. P var.
AI    Tuc    In the region of the Small Magellanic Cloud. SMS
             non-member. In the region of the globular cluster NGC 362.
             P var.
AK    Tuc    In the region of the Small Magellanic Cloud. SMS
             non-member. P var.
AL    Tuc    In the region of the Small Magellanic Cloud. SMS
             non-member.
AM    Tuc    The elements should be checked.
             [Fe/H] = -1.82. Delta(S) = 9.9.
AO    Tuc    The elements need improvement. Delta(S) = 5.
AP    Tuc    In the region of the Small Magellanic Cloud. SMS
             non-member.
AQ    Tuc    In the region of the Small Magellanic Cloud. SMS
             non-member.In the region of the globular cluster 47 Tuc.
             Min II 10.48.
AR    Tuc    In the region of the Small Magellanic Cloud. SMS
             non-member.
AU    Tuc    In the region of the Small Magellanic Cloud. SMS
             non-member.
AV    Tuc    In the region of the Small Magellanic Cloud. SMS
             non-member.
BD    Tuc    In the region of the Small Magellanic Cloud. SMS
             non-member.
BE    Tuc    In the region of the Small Magellanic Cloud.
BF    Tuc    In the region of the Small Magellanic Cloud. [A/H] = -0.7.
BG    Tuc    In the region of the Small Magellanic Cloud. SMS
             non-member.
BH    Tuc    In the region of the Small Magellanic Cloud. VB A
             (B 14.28m, 10" n).
BS    Tuc    (k - b)2 = 0.10.
BZ    Tuc    P var. Max = 2429849.448 + 127.78d*E (JD2410000 -
             35100) [03641]; Max = 2441193.541 +127.27d*E
             (JD2435100 - 43500) [A.M. van Genderen, AsAp Suppl 52,
             423, 1983]; since JD 2443500 - see Table.
CF    Tuc    In the region of the Small Magellanic Cloud. SMS
             non-member. Soft X-ray source. Distortion
             wave. Delta(m) = 0.057m [10065]. Min II 7.52.
DX    Tuc    Type RRC: is also possible.
tet   Tuc    For the period of the main oscillation (A = 0.0132m) see
             Table. Other instable frequences were also noted.
R     UMa    Maser (H2O).
S     UMa    S 1.5/6 e. P var. Max = 2398325 + 224.51d*E
             (JD2394000 - 2405000); Max = 2405290 + 230.20d*E
             (JD2405000 - 10500); Max = 2417530 + 223.96d*E
             (JD2410500 - 23500); Max = 2426324 + 228.53d*E
             (JD2423500 - 28800); since JD2428800 - see Table.
T     UMa    Maser (H2O).
W     UMa    ADS 7494 A (B 12.35m, 6.5", 44deg, 1963).
             dI = 0.037P; Min II 8.43, dII = 0.028P.
             Soft X-ray source. LX/Lbol = 1.7*10**(-4).
             P var. Min I = 2420980.8093 + 0.333638880d*E
             (JD2416000 - 21000); Min I = 2420980.8093 +
             0.333636993d*E (JD2421000 - 33000) [01760];
             Min I = 2435918.4169 + 0.33363832d*E (JD2433000 - 41000)
             [05327]; since JD2441000 - see Table. The light curve shape,
             including depths of minima, var. A moving wave with
             Delta(m) = 0.025m y and P ~1100d [10067] was noted. A
             flare (Delta(m) = 1.5m, lambda 3300 A,
             delta(lambda) = 50 A, JD2438511.7,
             delta(t) = 7 min) was announced [05788]. The system
             contains gaseous streams, dark spots on the surface of
             the components. H and K CaII emission.
Z     UMa    Usually 2 Max and 2 Min during a cycle.
RV    UMa    P var. Max = 2417861.434 + 0.4680618d*E
             (JD2417800 - 25000); Max = 2425053.675 + 0.4680654d*E
             (JD2425000 - 29000) [00188];
             Max = 2438459.945 + 0.468062d*E (JD2429000 - 40000) [03506];
             since JD2440000 - see Table. Blazhko effect, Pi = 92.12d
             (JD2436229 - 38114) [09835]. Pi var. [Fe/H] = -1.04;
             Delta(S) = 3.5.
RW    UMa    DI < 0.08P; Min II 10.34, DII = 0.10P.
             [Fe/H]A = -0.1, [Fe/H]B = -1.0. P var?
             Distortion wave, A = 0.11m V.
SU    UMa    The cycle of normal maxima 5d - 35d [09782, 03791].
             Three different mean values of the mean cycle of
             supermaxima change each other being active at different
             time intervals: P1 = 161.5d; P2 = 203.9d; P3 = 248.1d
             (<P> = 201.7d) [09276]. Porb = 2.06d/N (N = 26, 27, 28)
             or 3.1h. Surrounded by a faint halo (28' diameter) of soft
             X-ray sources.
SW    UMa    SB. Superior conjunction of the accretion disc
             T = 2445376.8601 + 0.0567433d*E [09836].
SX    UMa    P var strongly. Before JD2418800
             Max = 2416200.486 + 0.3071148d*E;
             Max = 2418800.213 + 0.3071345d:*E (JD2418800 - 22500)
             [00001]; Max = 2422653.5032 + 0.30711855d*E
             (JD2422500 - 26000) [10083]; Max = 2426400.418 +
             0.3071555d*E (JD2426000 - 29500); Max =
             2430000.250 + 0.3071301d*E (JD2429500 - 34000),
             Max = 2438508.751 + 0.3071363d*E (JD2434000 - 39000);
             since JD2441500 - see Table. [Fe/H] = -1.82,
             Delta(S) = 9.9.
SZ    UMa    mu alpha = -0.4853s, mu delta = +0.148".
TU    UMa    P var [03506]. [Fe/H] = -1.05, Delta(S) = 7.6.
TW    UMa    d = 0.002P; Min II 12.3:.
TX    UMa    Min II 7.13. P var. Min I = 2416426.801 + 3.063297d*E
             (JD2416000 - 22000); Min I = 2427926.492 + 3.063337d*E
             (JD2424200 - 30000); Min I = 2433440.431 + 3.063300d*E
             (JD2430000 - 38000) [09839]; since JD2438000 - see Table.
TY    UMa    P var, non-linear term: +6.4d*10**(-11)*E**2.
             dI = 0.05P, dII = 0.00P. The light curve shape var.
             12.10 <= Min I <= 12.14, 12.06 <= Min II <= 12.12.
UX    UMa    The shape of the eclipse light curve, the
             mean level of light outside eclipses, the depth of
             Min var. Deviations from the tabulated elements may
             reach  +-0.002d. Rapid brightness oscillations
             (28.54s <= P <= 30.02s) are sometimes observed [07304].
             Soft X-ray source.
UY    UMa    Min II 12.9.
VV    UMa    Min II 10.26. P var. Min I = 2439245.408 + 0.6873793d*E
             (JD2425600 - 40200) [09843]; Min I = 2440768.6280 +
             0.687367d*E (JD2440200 - 42700); since JD2442700 - see
             Table.
VX    UMa    Maser (H2O).
WX    UMa    Mu alpha = -0.4094s, mu delta = +0.955", VB B
             (A = BD +44deg 2051, dM2, 8.74m V; B 28", 133deg;
             common mu). Soft X-ray source. LX/LV = 0.095.
XY    UMa    Mu alpha = -0.0055s, mu delta = -0.175". P var.
             Non-linear term:  +2.77d*10**(-11)*E**2.
             The brightness outside eclipses var by 0.16m V. The depth
             of Min I is 0.48m - 0.67m, that of Min II is 0.19m.
             Migrating wave.
XZ    UMa    Min II 10.2. P var? Min = 2444986.445 + 1.2223105d*E
             (JD2414990 - 45000); since JD2445000 - see Table.
AA    UMa    Min II 11.53, Max II 10.94. The elements should
             be checked.
AC    UMa    VB B (A = BD  + 65G671, 9.97m V, B-V = +0.50m; B 19",
             114deg, 1957). The chart in [08953] is wrong.
AD    UMa    Blazhko effect is possible. Pi = 35d - 40d,
             delta(A) = 0.2m.
AE    UMa    The fundamental mode P0 is given in the Table.
             P1 = 0.066527d, Pbeat = 0.293616d [09869].
             Max 10.86 - 11.10, Min 11.46 - 11.52.
AF    UMa    d = 0.05P.
AK    UMa    The elements need improvement.
AN    UMa    The epoch of Min for periodic (P = Porb) light variations
             with A <= 1m B is given. Min II is present. B - V = 0.0
             in Max light,  +0.5 during an eclipse; U - B = -1.1.
             Circular polarization in B light -9% to -35%; linear
             polarization 0% - 13% with a sharp Max near Max light.
             Rapid changes (A = 0.03m, f = 0.4 - 0.8 Hz). The mean
             light level and the light curve shape var. During the low
             state (B ~19m) the light variability with porb disappears,
             emission lines occur only during 10% of Porb, IR excess is
             noted. Soft X-ray source, var. Emissions of H, HeI,
             He II, NIII, FeII.
AW    UMa    dI = 0.06P:; Min II 7.08, dII = 0.11P.
             The light curve shape var.
             P var. Min I = 2442150.4385 + 0.43873234d*E
             (JD2438000 - 42200); since JD2442200 - see Table.
AX    UMa    P var. Max = 2435951.354 + 0.53510d*E (JD2435900 - 38200)
             [04375]; during JD2445000 - 45900 - see Table.
BE    UMa    d = 0.006P. Outside eclipses var
             14.8m <= B <= 16.0m (reflection effect). The depth of
             eclipses for lambda lambda 3330 - 3700 A is greater than
             4.3m,that for lambda lambda 5265 - 6005 A is 1.5m.
BG    UMa    Min II 10.93. Alternative type EW.
BH    UMa    Min II 12.3.
BI    UMa    Min II 15.8.
BK    UMa    [Fe/H] = -1.29, Delta(S) = 6.6.
BL    UMa    Min II 16.2.
BM    UMa    The depth of Min II 0.80m.
BN    UMa    [Fe/H] = -1.65, Delta(S) = 8.9.
BP    UMa    D <= 0.04P. The elements need confirmation.
CE    UMa    In the region of the cluster of galaxies Abell 1213.
             SN 1966 omicron?
CF    UMa    Groombridge 1830 B (A = BD +38deg 2285, V = 6.45m,
             B - V = +0.75m, G8 subdwarf, mu alpha =  + 0.339s,
             mu delta = -5.81"; B 2", 165deg). A possible flare on
             February 27, 1968. A brightening of the combined light by
             0.6m pg on April 27, 1939 [09881]. Maybe the object does
             not exist [09882].
CH    UMa    X-ray source 1E 1003 +67. LX/Lopt = 0.04.
CM    UMa    P var?
CQ    UMa    The epoch of Max in U and B light
             coinciding with that of Min in V light is given.
             A(U) = 0.06m, A(B) = 0.06m.
CR    UMa    The elements for Max in U light are given. In B and V
             bands no periodicity is apparent. A(U) = 0.03m.
CW    UMa    Mu = 0.27", P = 300deg.
DF    UMa    ADS 8242A (B 11.4m, 1.8", 60deg, 1960).
             The data for combined brightness are given in the Table.
             SB1, Porb = 1.033824d. Mu alpha =  +0.0131s,
             mu delta = -0.038". Besides rapid variations (<V> = 10.14m,
             Delta(V) = 0.05m), long term variations are possible.
DG    UMa    Blazhko effect is possible.
DK    UMa    Soft X-ray source, lg Lx/Lv = -3.5. [Fe/H] = -0.38.
DL    UMa    Eclipses with P = 0.42d [04706].
DM    UMa    SB1 (Porb = 7.492d).
             Min = 2444026.97 + 7.478d*E (1979 - 1982);
             1981 - 1984 - see Table. Two Min in the light curve in
             1981 - 1982.
DN    UMa    ADS 8347 ABC (A 7.2m vis; B 9.0m vis, 0.121", 142.0deg,
             1981.5; C 8.3m vis, 4.0", 42deg, 1980; D = BS 4561,
             A1pCrEuSr:, V = 7.03m, B - V = +0.01m, 63.0", 114deg).
             The range of combined brightness for the three components
             is given. It is not known which of the components varies.
             The component D was used as a comparison star.
             Min II 6.73, Min II - Min I = 0.504P.
GM    UMa    SB, discrepant Porb = 3.2424d.
HH    UMa    Type EW: is also possible.
HN    UMa    Type DSCT: is also possible.
HU    UMa    VB A (B = GSC 3014.0222 = L265-581, 24", 250 deg, common proper
             motion).
II    UMa    Type RR: is also possible.
eps   UMa    SB (P=4.15A). Interferometric binary? (0.053", 94.5deg,
             1975.4). In 1976 - 1983 attempts to resolve the binary
             interferometrically were not successful.
             In the UMa moving cluster; mu alpha = +0.0131s,
             mu delta = -0.010".
ups   UMa    ADS 7534 A (B 11.5m, 11.3", 295deg, common mu).
             mu alpha = -0.0382s, mu delta = -0.156". The light curve
             shape and A var.
R     UMi    H2O maser.
S     UMi    P var. Max = 2422604 + 321.9d*E (JD2413000 - 23000);
             Max = 2432200 + 331.5d*E (JD2423000 - 32800);
             Max = 2436080 + 322.5d*E (JD2433000 - 37000);
             Max = 2439011 + 326.5d*E (JD2437000 - 41500);
             since JD2441500 - see Table.
T     UMi    P var. Max = 2428332 + 315.48d*E (JD2416500 - 29500);
             Max = 2436415 + 310.05d*E (JD2429500 - 37200);
             Max = 2442389 + 315.5d*E (JD2437200 - 43600); since
             JD2443600 - see Table.
U     UMi    P var. Max = 2416975 + 323.1d*E (JD2416500 - 21000);
             Max = 2428804 + 331.3d*E (JD2421000 - 29780) [00001];
             Max = 2429789 + 320.6d*E (JD2429780 - 34600) [00960];
             Max = 2434600 + 331d*E (JD2434600 - 36300);
             Max = 2437853 + 322.6d*E (JD2436300 - 39000); since
             JD2439000 - see Table.
V     UMi    Mean brightness var with P2 = 760d.
W     UMi    Min II 8.66; d = 0.02P. P var? Non-linear term in the
             elements is possible: -7.7d*10**(-10)*E**2.
X     UMi    P var? Max = 2424224 + 343d*E (JD2423800 - 25100)
             [00684]; since JD2438100 - see Table.
RR    UMi    SB (Porb = 749.4d [09896]).
RT    UMi    Min II 10.86.
RU    UMi    Min II 10.20.
RZ    UMi    Min II 13.5.
SZ    UMi    Variability needs confirmation.
alf   UMi    VB A (B 8.20m, F3V, 18.3", 218deg); SB1 (Porb = 10969d,
             E = 0.655 [09904]). P var. There is a non-linear term in
             the elements: +1.9877d*10**(-7)*E**2. The amplitude of
             light and radial velocity variation decreased in 1982.
             A(V) = 0.04m (1984).
gam   UMi    P var. Max = 2424301.78 + 0.14335d*E [10097]; Max =
             2427904.468 + 0.14335d*E [10098]. Elements given in the
             Table represent observations in 1964 - 1968. According to
             [09906] Vr var in 1922 with P = 0.108449d.
eps   UMi    VB A (B 12.5m, 76.9", 3deg). Min II 4.21.
S     Vel    Min II 7.83; d = 0.041P. P var? There is a non-linear term
             in the elements given in the Table: +4.47d*10**(-9)*E**2.
W     Vel    P var. Max = 2415053 + 384.3d*E (JD2414600 - 17400);
             Max = 2426080 + 399.9d*E (JD2422400 - 27300);
             Max = 2429990 + 388.0d*E (JD2427300 - 30100);
             Max = 2438328 + 398.7d*E (JD2430100 - 38800);
             since JD2438800 - see Table. OH emission.
Y     Vel    P var. Max = 2415900 + 438.6d*E (JD2411500 - 15900);
             Max = 2419930 + 447.7d*E (JD2415900 - 19930);
             Max = 2425755 + 452.8d*E (JD2421600 - 27600);
             Max = 2434150 + 439.5d*E (JD2427600 - 34200);
             since JD2434200 - see Table.
Z     Vel    P var. Max = 2415445 + 435.96d*E (JD2415000 - 25100);
             Max = 2425462 + 417.99d*E (JD2425100 - 29700) [00960];
             since JD2429200 - see Table.
RR    Vel    Min II 10.9.
RS    Vel    P var. Max = 2410403 + 421d*E (JD2410400 - 16800)
             [09961]; since JD2415450 - see Table.
RU    Vel    VB A (B 12m sf). According to [00017],
             Max = 2414390 + 63d*E.
RW    Vel    P var. Max = 2413553 + 430.4d*E (JD2413500 - 18500);
             Max = 2420610 + 465.7d*E (JD2418500 - 25700); since
             JD2425700 - see Table.
RX    Vel    Min II 10.5.
RY    Vel    [A/H] = -0.3. P var. Max = 2440246.67 + 28.1270d*E
             (JD2419000 - 40250) [05366]; since JD2443900 - see Table.
SW    Vel    P var. Max = 2434872.95 + 23.473d*E - 3.75d*10**(-5)*E**2
             (JD2412500 - 35500) [09636]. Since JD2440700 - see Table.
SX    Vel    The light curve has double maximum. The epoch of
             the primary (second) maximum is given in the Table.
TT    Vel    Min II 10.7.
UW    Vel    In the region of the open cluster NGC 3033.
YZ    Vel    Min II 12.8; DII = 0.040P; Min II - Min I = 0.537P.
ZZ    Vel    Min II 10.0.
AA    Vel    Min II 9.9.
AC    Vel    Min II 9.11.
AF    Vel    (k - b)2 = 0.06. Blazhko effect is possible [10110].
AH    Vel    SB? [10111]. In the region of the open cluster
             Collinder 173.
AI    Vel    Mu = 0.11", P = 76deg; (k - b)2 = 0.23.
             Light oscillations with the period P0 given in the Table
             are superimposed by oscillations with P1 = 0.08620868d and
             twice smaller amplitude. According to [10112] P0 is
             constant, P1 is increasing.
AK    Vel    In the region of the open cluster Collinder 173.
AL    Vel    d = 0.072P.
AO    Vel    In the region of the open cluster Collinder 173.
             Min II 9.55:. There is apsidal line motion.
             There is a sinusoidal term in the elements given in the
             Table: +0.058d*sin(phi), where phi = 2pi(E - 5338)/11500,
             and E values are counted from JD2415810.66.
             Min II = 2424270.125 + 1.5845993d (E - 5338) -
             -0.058d*sin(phi); Min II - Min I = 0.792d - 0.116d*sin(phi).
AP    Vel    P1 = 2.19984d; P1/P0 = 0.703. M - m var (0.25P <= M - m <=
             <= 0.50P) [03710].
AQ    Vel    d = 0.05P. The depth of Min II 0.05m.
AS    Vel    Min II 8.4; Min II - Min I = 0.55P.
AT    Vel    d = 0.03P. In the region of the open cluster Collinder 173.
AU    Vel    In the region of the open cluster Collinder 173.
AV    Vel    In the region of the open cluster Collinder 173.
AW    Vel    In the region of the open cluster Collinder 173.
AX    Vel    The first overtone mode light variation elements with the
             period P1 are given in the Table; the amplitude of
             the first overtone mode light variation A1 exceeds
             that of the fundamental mode, A0:A1(V) = 1.5A0(V).
             For the fundamental mode P0 Max hel = 2443878.885 +
             3.673174d*E.
             P1/P0 = 0.706; M - m var: 0.24P <= M - m <= 0.50P:.
AY    Vel    Min II 9.7.
AZ    Vel    Min II 13.0. In the region of the open cluster
             Collinder 173.
BB    Vel    P < 20d. In the region of the open cluster Collinder 173.
BC    Vel    Min II 12.3.
BD    Vel    d = 0.04P.
BE    Vel    Min II 12.5.
BF    Vel    The depth of Min II 0.04m.
BM    Vel    Min II 13.0. In the region of the open cluster NGC 2547.
             In the region of the open cluster Collinder 173.
BO    Vel    Min II 14.2.
BP    Vel    Min II 13.7.
BR    Vel    The shape of the light curve varies.
BT    Vel    Min II 14.8.
BU    Vel    Min II 10.96; Min II - Min I = 0.522P. In the region
             of the open cluster Collinder 173.
BV    Vel    In the region of the open cluster Collinder 173.
BW    Vel    Min II 14.3.
BX    Vel    In the region of the open cluster Tr 10.
BZ    Vel    Min II 10.4; Min II - Min I = 0.57P.
CK    Vel    D ~0.3d.
CL    Vel    Min II 13.4.
CR    Vel    d = 0.05P.
CS    Vel    [A/H] = 0.1. Possible member of the open
             cluster Ruprecht 79.
CU    Vel    The period of superhumps ~0.08d, A = 0.4m [10115].
CV    Vel    Min II 7.17.
CW    Vel    d = 0.024P. The depth of Min II 0.1m pg.
CZ    Vel    Min II 11.1.
DF    Vel    Min II 13.4.
DH    Vel    Min II 13.7.
DK    Vel    VB A (B 12.50m, 22", 315deg; C 16m, 10", 60deg).
DL    Vel    Min II 12.1.
DM    Vel    P = 123d?
DQ    Vel    Min II 11.0.
DS    Vel    Min II 10.8.
DT    Vel    (k - b)2 = 0.24.
DX    Vel    Min II 10.3. In the region of the open cluster Col 213.
EH    Vel    Min II 13.4.
EL    Vel    In the region of the open cluster Collinder 173.
EO    Vel    Min II 11.90, DII = 0.07P.
             Apsidal motion: Min II - Min I = 3.15d + 0.00003d*E.
             Min II = 2441716.75 + 5.32969d*E.
EP    Vel    In the region of the open cluster IC 2395.
ES    Vel    Min II 12.7.
ET    Vel    Min II 12.1.
EU    Vel    Min II 13.8.
EY    Vel    d = 0.04P:.
FM    Vel    Min II 12.9.
FS    Vel    Delta(S) = 10.
FT    Vel    Min II 10.5.
FW    Vel    Min II 10.0.
FX    Vel    Min II 10.5. The shape of the light curve varies.
FY    Vel    Min II 7.03. Type ELL? [06827].
FZ    Vel    VB A (B 12.08m, 24.2", 338deg).
GG    Vel    VB A (B 11.2m, 6", delta(alpha) = 0). P = 2.950432d?
GP    Vel    <Min II> 6.90. Min II - Min I = 0.55P.
             The shape of the light curve varies.
             There are probably long-period light
             oscillations: Min = 2442681.6 + 93.3d*E (A ~0.02m)
             [10051]. The period of X-ray pulses var: 282.8913s
             (1975.5) [10125]; 282.919s (1975.7) [10126]; 282.869s
             (1976.4), 282.838s (1976.9) [10127]; 282.80s (1978.9)
             [10128]; 282.745s (1979.3), 282.7874s (1980.3), 282.87s
             (1981.0) [10129]; 282.93s (1981.9 - 1982.9); 282.9306s
             (1983.2) [10078].
GV    Vel    In the region of the open cluster NGC 2660.
HU    Vel    Pulsar PSR 0833-45. In the nebula Vela SNR.
             Star M [08276]. The pulsed radiation varies in radio,
             optical and gamma rays with P = 0.089s.
             P var [10136 - 10139]: P = 0.089233318274s
             (JD2442553 - 680), P = 0.089234713929s (JD2442700 - 848),
             P = 0.089244007685s (JD2443654 - 676), P = 0.089245406487s
             (JD2443719 - 850) [10137]; P = 0.089256985348s
             (JD2444795.84) [10138].
HV    Vel    A member of the open cluster IC 2391.
HW    Vel    P = 0.26133d? A member of the open cluster IC 2391.
HX    Vel    VB A (B 7.1m, 0.3", 313deg, 1949); in the region
             of the open cluster IC 2395. Min II 5.50:.
HY    Vel    VB A (B 5.7m, 76.6"); a member of the open cluster IC 2391.
             Min II 4.90.
IL    Vel    A var (0.02m <= A <= 0.15m). Beat period 10.075d
             (Min A = 2443175.5 + 10.075d*E).
IM    Vel    VB A (B 9.73m, 3.3", 179deg, 1948).
             The double wave of light variations
             with rotation period Prot = 2.85204d and A = 0.03m is
             superimposed by oscillations with the periods
             P1 = 0.00812815d (A1 = 0.0043m), P2 = 0.00808206d
             (A2 = 0.0035m), P3 = 0.00810503d (A3 = 0.0008m), P4 =
             0.004052519d (A4 = 0.0009m), P5 = 0.004064065d
             (A5 = 0.0004m), P6 = 0.004041031d (A6 = 0.0004m),
             P7 = 0.00815128d (A7 = 0.0004m) [09208].
IN    Vel    P = 65 - 70d,
IP    Vel    VB A (B 11.2m V, 2.1", 200deg, 1929). P > 1.25d.
IQ    Vel    Min II 12.94; Min II - Min I = 0.500P.
IS    Vel    A(U) var: 0.005m <= A(U) <= 0.018m.
IT    Vel    Min II 7.08. P = 23.52d?
OQ    Vel    The type is doubtful.
V0360 Vel    Several close companions.
gam 2 Vel
             VB A (B 4.22m, 41.3", 220deg).
             SB2 (Porb = 78.5002d [10119]). In HII region.
             T0 = 2433633.0 is the epoch of the conjunction where the
             O component is in front [10119].
lam   Vel    VB A (B 14.8m, 18.2", 137deg).
omi   Vel    A member of the open cluster IC 2391. P(VR) = 2.74d.
             P = 2.76d? SB1? The epoch of the light maximum is given.
             Close binary system?
R     Vir    P var. Max = 2381914 + 145.77d*E (JD2338900 - 2402000);
             Max = 2402321 + 144.90d*E (JD2402000 - 18000);
             Max = 2418268 + 145.48d*E (JD2418000 - 30000);
             Max = 2430489 + 148.32d*E (JD2430000 - 34000);
             Max = 2434193 + 144.63d*E (JD2434000 - 38500);
             Max = 2438829 + 147.45d*E (JD2438500 - 43000);
             since JD2443000 see Table. Maser (SiO).
S     Vir    P var. Max = 2399014 + 374.7d*E (JD2398600 - 2405000);
             Max = 2412970 + 376.2d*E (JD2412000 - 23500, on average);
             Max = 2423502 + 381.52d*E (JD2423500 - 23000); since
             JD2433000 - see Table. Maser (H2O, SiO).
T     Vir    Maser (OH, H2O, SiO).
V     Vir    P var. Before JD2427000 Max = 2400467 + 250.17d*E;
             Max = 2427225 + 246.54d*E (JD2427000 - 31500);
             since JD2431500 - see Table.
W     Vir    The epoch of Min is given. P var.
             Min = 2404151.168 + 17.2707d*E (JD2403000 - 23200);
             Min = 2423200.837 + 17.2634d*E (JD2423200 - 29700);
             since JD2429700 - see Table. The light curve shape var.
             [Fe/H] = -1.03.
X     Vir    VB A (B 12m, dK4, 0.6', ~50deg). The brightenings
             of 1871 and 1882 may be due to misidentification [01651].
Z     Vir    mu alpha = +0.0098S, mu delta = -0.120".
             P var. Max = 2409683 + 309.19d*E (JD2408000 - 18500);
             since JD2418500 - see Table.
RS    Vir    Maser (OH, H2O, SiO). P var. Max =2412592 + 351.29d*E
             (JD2412000 - 31000); since JD2431000 - see Table.
RT    Vir    Maser (OH, H2O, SiO). According to [10145], observations
             of 1970-1977 are not in agreement with the P value in the
             Table.
RU    Vir    P var? Max = 2425120 + 435.9d*E (JD2414000 - 31500); since
             JD2431500 - see Table.
RV    Vir    P var. Max = 2412272 + 268.39d*E (JD2412000 - 31500);
             since JD2431500 - see Table.
RX    Vir    VB (B 13.0m vis, 1.1", 107deg, 1939). According to
             photoelectric observations [06450, 08837], 8.72m - 8.81m V.
             Const? [06450].
SS    Vir    P var. Max = 2415910 + 352.75d*E (JD2415900 - 21500);
             Max = 2421913 + 361.7d*E (JD2421500 - 26500);
             Max = 2428359 + 350.12d*E (JD2426500 - 40000);
             since JD2440000 - see Table.
ST    Vir    P var. Max = 2425005533 + 0.4108494d*E (JD2422000 - 29100)
             [10146]; Max = 2436702.513 + 0.4108168d*E
             (JD2433000 - 39000) [03415]; since JD2439000 - see Table.
             Blazhko effect? Delta(S) = 0.8.
SU    Vir    P var. Max = 2415040 + 213.7d*E (JD2415000 - 19500);
             Max = 2419926 + 210.96d*E (JD2415000 - 31500);
             Max = 2437378 + 210.2d*E (JD2431500 - 38500);
             since JD2438500 - see Table.
SV    Vir    P var? The mean elements are given. Maser (H2O).
SZ    Vir    Possibly EW with a very small A.
TV    Vir    VB A (B P).
TW    Vir    Porb = 0.182666d [09430]. Variability of ellipsoidal
             character in H light: P = Porb/2, A(H) = 0.13m.
             X-ray source.
TX    Vir    VB A (B 15m, 0.3' P).
TY    Vir    [Fe/H] = -1.7.
TZ    Vir    P2 = 6900d is superimposed?
UU    Vir    [Fe/H] = -0.3. delta[S] = 0.7.
UW    Vir    d = 0.011P. P var. Min = 2419942.513 + 1.8106818d*E
             (JD2415000 - 34500); since JD2441000 - see Table
UY    Vir    d = 0.014P; Min II 8.1.
VV    Vir    Min II 12.2:.
VW    Vir    SN 1895 (NGC 4424).
XX    Vir    [Fe/H] = -1.5. Delta(S) = 9:.
YZ    Vir    [A/H] = -0.9.
AD    Vir    P var. Max = 2425259.259 + 0.5522109d*E
             (JD2419000 - 31000); since JD2431000 - see Table.
AF    Vir    P var. Max = 2429051.697 + 0.4838214d*E
             (JD2419500 - 36000); Max = 2436718.3758 +
             0.4838386d*E (JD2436000 - 37500) [10159];
             since JD2440000 - see Table. DM var.
AG    Vir    The depth of Min II up to 0.44m.
             The light curve shape and A var.
             dI = 0.03P:, dII = 0.66P. Min II - Min I = 0.512P.
             P var. Min = 2434487.4297 + 0.6426489d*E
             (JD2424500 - 34500); since JD2434500 - see Table.
AH    Vir    mu alpha = +0.0015S, mu delta = -0.111"
             ADS 8472 A (B 13.2m, 1.3", 17deg).
             The combined brightness is given,
             dI = 0.07P. The depth of Min II 0.53m, dII = 0.00P.
             The light curve shape var.
             P var. Min = 2434841.3963 + 0.40751843d*E
             (JD2425000 - 35000) [05222]; Min = 2435573.710 +
             0.40752192d*E (JD2435000 - 41400); Min =
             2441411.460  +  0.40753186d*E (JD2441400 - 44000);
             since JD2444000 - see Table.
AK    Vir    VB B (A = BD -17deg 3996; B 44", 286deg).
AL    Vir    P var [A/H] = -0.7.
AN    Vir    P2 ~1000d is superimposed.
AO    Vir    VB A (B 11.4m vis, 6.9", 321deg, 1956, common
             Vr). delta(M) is possibly in error because of the
             companion. P var. Max = 2413949  +  256.88d*E
             (JD2412900 - 21000); since JD2421000 - see Table.
AS    Vir    P var. The Table gives the mean elements valid after
             JD2425600. Blazhko effect? [03506].
             (k - b)2 = 0.08.
AT    Vir    P var. Max = 2426831.367 + 0.5258053d*E
             (JD2420500 - 35000) [00188]; since JD2435000 - see Table.
             (k - b)2 = 0.00, Delta(S) = 6.0.
AU    Vir    [Fe/H] = -1.84, Delta(S) = 10.1.
AV    Vir    Delta(S) = 5.5.
AW    Vir    Min II 11.67.
AX    Vir    Min II 10.24.
AY    Vir    Maser (H2O).
AZ    Vir    Min II 11.37.
BB    Vir    Blazhko effect?
BC    Vir    P var. Max = 2419922.289 + 0.56451468d*E
             (JD2419900 - 30100); the Table gives current elements.
BD    Vir    P var. Min = 2424971.720 + 2.548410d*E
             (JD2424900 - 32000); since JD2432000 - see Table.
BF    Vir    Min II 10.72. Total eclipses.
             P var. Min = 2416595.67 + 0.64057d:*E (JD2414000 - 19000);
             Min = 2440331.809 + 0.64057631d*E
             (JD2426000 - 41000); since JD2441000 - see Table.
BH    Vir    Min II 10.24. Distortion wave?
             (Delta(V) = 0.04m).
BN    Vir    P var. Max = 2419865.422 + 0.39127585d*E
             (JD2419800 - 28300); since JD2432600 - see Table.
BO    Vir    P var. Max = 2419513.388 + 0.52005916d*E
             (JD2419500 - 33000); since JD2433000 - see Table.
BQ    Vir    P var?
BS    Vir    [Fe/H] = -1.84. Delta(S) = 10.1.
BV    Vir    P var. Max = 2426070.488 + 0.4965803d*E
             (JD2419900 - 28500); since JD2436600 - see Table.
BW    Vir    P var. Max = 2420247.403 + 0.4706660d*E
             (JD2420200 - 26800); since JD2426800 - see Table.
CG    Vir    Min II 10.9.
CK    Vir    [Fe/H] = -2.0.
CM    Vir    d = 0.05P. P var. Min = 2425411.330 + 3.40167d*E
             (JD2423900 - 28400) [00001]; during JD2432200 - 34200 - see
             Table.
CS    Vir    The epoch of Max in B light is given.
             SB (Porb = 1618d). IR excess (4.8 mkm).
CU    Vir    ADS 9152 A (B 11.9m, G1V, 60", 212deg).
CW    Vir    The epoch of min is given.
CX    Vir    The depth of Min II 0.30m.
DK    Vir    According to [10189], P1 = 0.1162d, P2 = 0.1086d.
             (k - b)2 = 0.20.
DL    Vir    SB (Porb = 2286d).
             The spectrum shows the A-component of the eclipsing
             system and the G8III star around which the eclipsing
             system is orbiting.
DM    Vir    Min II 9.49. DII = DI.
DN    Vir    P >= 100d.
DT    Vir    Mu alpha = -0.044s, mu delta = -0.02". SB?
             Rotation period 1.535d [10014], A = 0.05m V.
DV    Vir    Blazhko effect?
EF    Vir    According to [04784], const?, 16.1m pg.
EP    Vir    IR excess (4.8 mkm).
EQ    Vir    SB; [Fe/H] = -0.08; mu alpha = -0.018s, mu delta = -0.09".
             Min = 2441129.585 + 3.914169D*E + 0.0001803345d*E**2,
             A = 0.10m V, M - m = 0.40P. Soft X-ray source,
             lg FX/FV = -2.07.
EW    Vir    P >= 100d.
EX    Vir    P >= 100d.
EY    Vir    P >= 100d.
FF    Vir    The P value for magnetic field variations is given.
FG    Vir    ADS 8471 A (B 13.51m, 25", 352deg, 1909;
             C 11.85m, 74", 195deg, 1909).
FI    Vir    Mu alpha = +0.043s, mu delta = -1.22".
FL    Vir    VB AB (A = 0.76", P = 16A). Both components show flares?
             The range of combined brightness is given.
             Mu alpha = -0.118s, mu delta = +0.26".
FM    Vir    SB2, Porb = 38.324d.
FN    Vir    Mu alpha = -0.064s, mu delta = +0.28". SB?
             X-ray source, LX/Lbol = -3.55.
FO    Vir    Min II 6.67.
FQ    Vir    Deep Min II.
GG    Vir    Multiperiodicity, 0.023d <= P <= 0.083d, A <= 0.02m.
GH    Vir    P var.
GK    Vir    The secondary is a red dwarf (M0 - M6).
GL    Vir    Mu alpha = -0.087s; mu delta = +0.23".
GM    Vir    P ~1.6d/n.
GQ    Vir    Mu alpha = -0.045s, mu delta = -0.44".
GR    Vir    The depth of Min II 0.41m.
GU    Vir    P var. Max = 2439236.36 + 0.466562d*E
             (JD2438100 - 39300); during JD2441300 - 42600 - see Table.
LV    Vir    Type RR: is also possible.
MW    Vir    Type DSCTC: is also possible.
NN    Vir    Type EW: is also possible.
alf   Vir    The Table gives the epoch of Min for the ellipsoidal
             variability and Porb. The depth of Min II up to 0.08m.
             SB 2. e = 0.205 +- 0.004. Apsidal motion: Pi = 108a +- 5a.
             Pulsations: P var, P = 0.17378587d (1908 - 1956);
             since 1956 Max = 2445405.63 + 0.17378680d*E [10181]. A var.
             3 companions according to lunar occultation observations:
             3.1m, 0.0025"; 4.5m, 0.05"; 7.5m, 0.5". Soft X-ray source,
             LX/Lbol = 2.9*10**(-8).
psi   Vir    Binary? (lunar occultations).
R     Vol    P var. Max = 2415238 + 441d*E (JD2394100 - 2418800)
             [10143]; since JD2422700 - see Table.
S     Vol    P var. Max = 2415042 + 397.6d*E (JD2415000 - 24200),
             Max = 2428880 + 392.1d*E (JD2423000 - 28900),
             Max = 2434113 + 401.7d*E (JD2428900 - 34900),
             Max = 2434910 + 387.2d*E (JD2434900 - 39200);
             since JD2439200 - see Table.
T     Vol    P var. Max = 2413135 + 189.8d*E (JD2413100 - 14600);
             Max = 2416870 + 171.8d*E (JD2414600 - 16900);
             Max = 2416870 + 176.8d*E (JD2416800 - 24400);
             Max = 2424460 + 170.8d*E (JD2424400 - 27200);
             Max = 2429925 + 182.3d*E (JD2427200 - 30000);
             since JD2440000 see Table.
RX    Vol    P < 20d?
ST    Vol    SP component of a very close pair.
SV    Vol    The shape of the light curve varies.
TX    Vol    Min II 10.5. P var. Min I = 2416789.869 + 5.38845d*E
             (JD2415100 - 26000), Min I = 2431150.345 +
             5.3887d*E (JD2426000 - 31400), Min I =
             2433542.609 + 5.388d*E (JD2431400 - 33600)
             [00001]; since JD2433600 see Table.
R     Vul    P var. Max = 2400169 + 138.3d*E (JD2400100 - 02700),
             Max = 2402779 + 136.76d*E (JD2402700 - 19800),
             Max = 2419880 + 137.45d*E (JD2419800 - 24400),
             Max = 2424413 + 136.76d*E (JD2424400 - 28500
             [00960]; Max = 2429331 + 135.9d*E (JD2428500 - 32000)
             [00001]; since JD2432000 see Table.
S     Vul    In the region of the open cluster C 1947 + 272 [10123].
             P var. Max = 2401772 + 67.37d*E (JD2401760 - 6400),
             Max = 2408180 + 67.70d*E (JD2408170 - 14950),
             Max = 2415285 + 68.26d*E (JD2415300 - 22800),
             Max = 2423468 + 67.72d*E (JD2423450 - 27200),
             Max = 2428227 + 68.18d*E (JD2428220 - 31300)
             [00761]; Max = 2432775 + 67.51d*E (JD2431300 - 34500)
             [10148]; Max = 2437150 + 68.66d*E
             (JD2436800 - 39600), Max = 2441507 + 67.344d*E
             (JD2439600 - 43000) [10124]; since JD2443000 see Table.
             [A/H] = 0.1.
T     Vul    P var. Max = 2419372.151 + 4.435589d*E (JD2409880 - 34000);
             since JD2434000 see Table.
V     Vul    Min II 8.65. P var. Min I = 2414912.9 + 74.96d*E
             (JD2414900 - 20840),  Min I = 2420909.8 + 75.686d*E
             (JD2420900 - 24810), Min I = 2425072.9 + 76.344d*E
             (JD2425050 - 30000), Min I = 2430023.5 + 75.957d*E
             (JD2430000 - 32500) [10149]. Study of period variation and
             changes of Min II by Min I see also in [00767, 010150].
W     Vul    In the region of the open clusters NGC 6882, NGC 6885.
X     Vul    P var. Max = 2420636.337 + 6.319301d*E (JD2417000 - 34000)
             [00768]; since JD2435000 - see Table.
Z     Vul    VB A (B 12.0m, 13", 359deg). Min II 7.58. P var. Min I =
             2425456.117 + 2.454926d*E (JD2413200 - 37000)
             [00063]; since JD2437000 - see Table.
RS    Vul    Min II 6.86; Min II - Min I = 0.508P.
RU    Vul    A var. P var. Max = 2416266 + 155.95d*E
             (JD2415000 - 36000), Max = 2436779 + 150.7d*E
             (JD2436000 - 38800), Max = 2438855 + 153.4d*E
             (JD2438800 - 41620), Max = 2441193 + 138.5d*E
             (JD2441620 - 42600); since JD2442600 - see Table.
RX    Vul    P var. Max = 2420301 + 438d*E (JD2418900 - 22500)
             [04018]; since JD2424700 - see Table.
RZ    Vul    Slow variations of mean brightness with P = 1410D and
             A = 2m are superimposed by fluctuations with the cycle
             40 - 100d and A up to 1m.
SU    Vul    In the region of the open cluster NGC 6882, NGC 6885.
SV    Vul    [Fe/H] = 0.23. P var. There is a nonlinear term in the
             elements given in the Table: -0.0001814d*E**2.
SX    Vul    In the region of the open cluster NGC 6940.
UU    Vul    The co-ordinates are wrong?
             [10156].
VV    Vul    Min II 12.1; d = 0.026P. P var. Min I = 2416670.527 +
             3.411224d*E (JD2416600 - 27500) [00134];
             since JD2426000 - see Table.
VW    Vul    Porb = 0.0731d [10160].
VY    Vul    Min II 14.4:.
WW    Vul    There is quasi-periodicity in light minima with the cycle
             404d.
XZ    Vul    Min II 11.4. P var. Min I = 2426477.525 + 3.0895116d*E
             (JD2416900 - 36000) [04427]; since JD2436000 - see Table.
AB    Vul    The depth of Min II 0.02m.
AD    Vul    Min II 0.010P.
AF    Vul    Min = 2436545.23  +  0.954d*E (JD2436200 - 900) [03148].
AR    Vul    In the region of the open cluster Stock 1.
AT    Vul    Min II 9.3; d = 0.02P.
AW    Vul    Min II 10.9; d = 0.020P.
AX    Vul    d = 0.018P.
AY    Vul    d = 0.020P. P var. Min hel = 2436128.388 + 2.4124239d*E
             (JD2418500 - 40700); since JD2440700 - see Table.
AZ    Vul    Min II 11.9.
BB    Vul    In the region of the open cluster NGC 6940.
BE    Vul    VB A (BC 11.92m, 50", 320deg). Min II 9.90. P var.
             Min I = 2426144.490 + 1.55205d*E
             (JD2426140 - 28880), Min I = 2430698.203 +
             1.5520442d*E (JD2430690 - 34660), Min I =
             2435340.373 + 1.552052d*E (JD2435340 - 40070);
             since JD2440100 - see Table.
BF    Vul    Elements given in the Table represent well only the bright
             maxima. The fainter maxima are represented by the elements:
             Max = 2427731 + 95.4d*E.
BI    Vul    Min II 14.86. P var? Min I = 2424759.70 + 0.251828d*E
             [00193]; since JD2444750 - see Table.
BN    Vul    Delta(S) = 7. P var. Max = 2414815.759 + 0.5941295d*E
             (JD2414000 - 30000) [00388]; Max = 2434244.333 +
             0.59412538d*E (JD2430000 - 36000) [00616];
             Max = 2438265.386 + 0.59412763d*E (JD2436000 -
             41000) [09009]; since JD2441000 - see Table.
BO    Vul    Min II 10.6. P var. Min I = 2429984.332 + 1.9459123d*E
             (JD2415000 - 30000) [00007]; Min I = 2432379.766 +
             1.9459206d*E (JD2427000 - 35000), since
             JD2435300 - see Table.
BP    Vul    Min II 10.5.
BS    Vul    Min II 11.10.
BT    Vul    d = 0.03P; Min II 12.3.
BU    Vul    P var. Min = 2431006.204 + 0.5689904d*E
             (JD2426500 - 31100) [00001];  since JD2433500 - see Table.
BV    Vul    S 6.5/6-.
BW    Vul    P var. Max = 2424000.171 + 0.20102229d*E
             (JD2424000 - 26500), Max = 2426500.079 +
              + 0.20102933d*E (JD2426500 - 31500), Max =
             = 2432000.054 + 0.20103513d*E (JD2431500 - 41000);
             since JD2441000 - see Table.
CD    Vul    Min II 11.9.
CK    Vul    Max 2331186:. Connected with nebulae. Type NR?
CS    Vul    Min II 13.6.
DR    Vul    Min II 9.19; DII = 0.132P.
             There is apsidal motion with the period 37.8 years.
             Elements given in the Table contain supplementary
             terms: -0.07165d*sin(0.05863deg*E) - 0.00269d*
             *sin(0.11726deg*E).
             Min II = 2440301.7934 + 2.2508645d*E + 0.07165d*
             *sin(0.05863deg*E) - 0.00269d*sin(0.11726deg*E).
             P var? [10185]. The depth of minima varies.
DY    Vul    VB A (B 13.0m V, 14", 300deg).
EH    Vul    P var. Max = 2429609 + 185d*E (JD2429600 - 30600);
             since JD2430800 - see Table.
EP    Vul    S 6.5/5.
EQ    Vul    Min II 12.5; Min II - Min I = 0.31P; DII = 0.050P,
             dII =  0.010P.
ER    Vul    P var. Min I = 2440182.2593 + 0.69809510d*E
             (JD2433100 - 40200) [08592]; since JD2440100 - see Table.
             7.35m <= Min II <= 7.44m. The shape of the light
             curve and depths of minima vary.
ES    Vul    VB A (B 10.1m, 1.6", 126deg).
ET    Vul    [A/H] = -0.4. P var. Max = 2425110.63 + 54.33d*E
             (JD2422900 - 26600), Max = 2432875.80 + 54.33132d*E
             (JD2432700 - 35430), Max = 2438656.99 + 53.81d*E
             (JD2436050 - 39035), Max = 2439253.55 + 54.24d*E
             (JD2439035 - 40990) [10168]; since JD2441900 - see Table.
EU    Vul    Min II 13.3.
EV    Vul    Min II 11.9. P var. Min I = 2428750.459 + 2.822084d*E
             (JD2428400 - 36400) [04027]; Min I = 2436748.37 +
             2.82220d*E (JD2436380 - 750) [03732]; since
             JD2441500 - see Table.
EX    Vul    d = 0.03P.
EY    Vul    The depth of Min II 0.05m.
FG    Vul    In the region of the open cluster NGC 6940. Star 120.
             The epoch of light minimum is given.
FH    Vul    P var. The elements given in the Table are valid since
             JD2436000.
FK    Vul    Blazhko effect.
FM    Vul    Min II 13.0.
FN    Vul    d = 0.02P; Min II 14.2.
FP    Vul    Min II 15.6.
FQ    Vul    Min II 12.9. Apsidal motion with P = 280 years. Correction
             of mispints in [04248] see in [04244].
FR    Vul    Probably the period must be doubled.
FS    Vul    Min II 15.2.
FU    Vul    sp component of a close pair.
FW    Vul    Min II 12.9.
FY    Vul    sp component of a close pair. Cycle 30 - 70d [04027].
FZ    Vul    Min II 13.9.
GG    Vul    P var. Max = 2427681.0 + 106.5d*E (JD2427500 - 28850);
             since JD2428850 - see Table.
GH    Vul    P = 2.5d?
GI    Vul    Min II 13.8.
GK    Vul    Red.
GN    Vul    Min II 12.4; d = 0.04P.
GO    Vul    Min II - Min I = 0.515P. The depth of Min II 0.03m.
GP    Vul    Min II 11.2; Min II - Min I = 0.48P.
GQ    Vul    nf component of a close triple group of stars.
             P var. Max = 2434399.825 + 12.647241d*E (JD2426100 - 38000)
             [04414]; since JD2444600 - see Table.
GR    Vul    Min II 13.3. The chart in [04244] is wrong.
GT    Vul    Min II 15.8.
GU    Vul    Min II 12.2.
GV    Vul    Probably the period must be doubled. Probably the period
             must be doubled.
HI    Vul    Min II 12.6.
HP    Vul    The depth of Min II 0.04m.
HS    Vul    Min II 14.2.
HU    Vul    Blazhko effect?
HV    Vul    P var. Max = 2437165.449 + 0.419906d*E (JD2437100 - 38670);
             since JD2438670 - see Table. Blazhko effect?
HW    Vul    P var. Max = 2429077.0 + 75.44d*E (JD2427190 - 29080),
             Max = 2429077.0 + 73.94d*E (JD2429070 - 32470);
             since JD2432350 - see Table.
IU    Vul    P var. Max = 2434656 + 320.2d*E (JD2432700 - 37860) [04427];
             since JD2437860 - see Table.
IW    Vul    Min II 13.1.
KN    Vul    Min II 13.4.
KO    Vul    Red.
KS    Vul    Very red.
LT    Vul    Multiperiodicity: P1 = 0.109414d, A1(V) = 0.0234m;
             P2 = 0.11094d, A2(V) = 0.0074m; P3 = 0.1215d,
             A3(V) = 0.0070m (JD2444054 - 096) [10173];
             P1 = 0.109621d, A1(B) = 0.0340m; P2 = 0.093528d,
             A2(B) = 0.0136m (JD2444071 - 465) [10193].
LU    Vul    Nova Vul 1968 N2.
LV    Vul    Nova Vul 1968 N1. VB A (B 18m, 6", 115deg).
LW    Vul    Min II 16.3.
MN    Vul    Min II 16.1; Min II - Min I = 0.518P; DII = 0.10P.
MO    Vul    Min II 14.8. P var?
MR    Vul    P2 = 111.0d?
MT    Vul    Multiperiodicity:
             P2 = 119.93d (A2 = 0.3m), P3 = 25.02d (A3 = 0.4m:).
MX    Vul    P = 181.8d?
NO    Vul    Min II 14.1.
NS    Vul    VB A (B 8.8m, A0, 0.73", 273deg, 1978.6),
             The range of combined light variation is given.
PS    Vul    VB A (B 10.0m, 0.4", 105deg, 1980.0); SB2.
PT    Vul    P1 = 256.12714s (A1 = 1.14%), Max1 =
             2445166.660914 HJED; P2 = 256.33205s (A2 = 1.09%),
             Max2 = 2445166.659424 HJED; P3 = 128.11496s (A3 = 0.37%),
             Max3 = 2445166.660024 HJED. mu = 0.1508", P=1.6deg.
PU    Vul    Pre-outburst SP M4 (1958). Gradual light increase in
             1977 - 79 up to 8.7m V; in 1979 A = 0.29M V,
             Min I = 2443943.39 + 78.12d*E [10197]. In the max of 1979
             Sp F5Ia - F8-9I. In February 1980 an abrupt light decrease
             started; the star reached V = 13.65m by early September.
             By September, 1981 the star recovered from the deep Min of
             500d duration. During the 1980 - 81 minimum Sp M5 with TiO
             bands, emissions of Halpha, NaD, [OII], FeII, rare earths.
             In 1982 - 84 8.35m - 8.87m V, Sp became F again. Simetimes
             Halpha, Hbeta emissions have been detected, often
             with P Cyg profiles.
V0398 Vul    Not identical to IRC+30416 = NSV 12861.
