Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.sai.msu.su/gcvs/gcvs/nl74/74nl_rem.txt Дата изменения: Mon Mar 15 06:27:16 1999 Дата индексирования: Sat Dec 22 06:44:20 2007 Кодировка: Поисковые слова: m 8

V0742 Cas| 940| SB, Porb = 55.9212d.
V0745 Cas| 1805| Component B of the double system observed brighter than in the Hipparcos Input Catalogue.
V0746 Cas| 1921| SB, Porb = 27.8d.
BC Scl| 2164| May be eclipsing.
V0747 Cas| 2271| VB. The variability may be due to the fainter component.
CL Cet| 2274| Type ELL: is also possible.
pi Cas| 3414| SB, Porb = 1.9642d.
BI Scl| 7330| Type E: is also possible.
V0547 Per| 8182| High proper motion (LTT 10610) not confirmed by HIPPARCOS data.
alf Tri| 8796| SB (Porb = 1.767 d).
V0369 And| 9150| VB (0".1, 128 deg, 1986.9).
V0374 And| 9867| Not identical with BD+44 422.
EE Cet| 13199| The variability may be due to the fainter (B) component.
CP Oct| 14700| Variability type and spectral type (F2/F3Ib/II) do not agree.
EL Cet| 14915| SB2.
V0580 Per| 17666| The variability may be due to the fainter (B) component.
CZ Cam| 18593| P = 267.79d, semiregular behavior unusual for B5 stars.
V0582 Per| 19335| A single deep minimum at the bottom of the small-amplitude (5.63 - 5.64) wave.
V1144 Tau| 20963| SB, Porb = 13.88d.
RX Cae| 21063| Variability type and spectral type (F3/F5II) do not agree.
V1148 Tau| 21575| Type LBV: is also possible. SB, Porb = 2.2075d.
V1152 Tau| 21810| Type E: with P = 11.080d is also possible.
V0592 Per| 22050| VB (0".2, 197 deg, 1989.7).
HV Eri| 22326| Type RRC: is also possible.
VW Pic| 23196| Variability may be due to component B.
VZ Pic| 24186| Kapteyn's star.
VW Col| 24710| Variability may be due to component B.
V1377 Ori| 26263| SB?, Porb ~ 5.5 to 6.5d.
V1161 Tau| 26282| Variability needs confirmation.
V0431 Aur| 26354| P = 16.86d detected in HIPPARCOS data.
V0433 Aur| 26606| SB?
V1380 Ori| 27309| In a bright nebula.
AN Men| 28440| Type RRC: is also possible.
IU CMa| 30426| Type LBV: is also possible.
V0741 Mon| 32839| Type ACV: is also possible.
QX Gem| 33166| Type ACV: is also possible.
V0360 Pup| 33864| Type ACV: is also possible.
V0750 Mon| 34116| In the region of the nebula IC 2177.
V0753 Mon| 34684| Type ACV: is also possible.
V0364 Pup| 34836| 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.
MO CMa| 35015| The amplitude can have been overestimated (M. Grenon, private communication).
tau CMa| 35415| SB, Porb = 154.90d.
BO CMi| 35776| Several episodes of outburst-like activity.
NO CMa| 35795| Type LBV: is also possible.
V0376 Pup| 36728| Type ACV: is also possible.
V0378 Pup| 36981| Type BE is also possible.
V0345 Gem| 37197| The variability may be due to the fainter (B) component.
V0393 Pup| 37925| SB, Porb = 2.5248d.
omi Pup| 38070| Type EA: is also possible.
V0419 Pup| 39637| Not a nearby star (despite having a Gl number).
CW Lyn| 42554| Type RRC: is also possible.
OQ Vel| 43071| The type is doubtful.
FV Cnc| 43199| The type is doubtful.
V0491 Car| 48665| Mean magnitude 9.69.
V0493 Car| 48832| SB, Porb = 3.368d.
V0498 Car| 49945| Type BE: is also possible.
GM UMa| 50097| SB, discrepant Porb = 3.2424d.
V0360 Vel| 53938| Several close companions.
HH UMa| 54165| Type EW: is also possible.
FL Leo| 54723| Variability range according to E.M. Halbedel, IBVS No. 3502, 1990.
HN UMa| 55030| Type DSCT: is also possible.
V0902 Cen| 55031| VB, rho = 12". Variability may be spurious.
V0534 Car| 55078| Flare-like activity.
V0915 Cen| 57067| The variability type is not quite consistent with the spectral type (B9II/III).
FX Leo| 57480| Not a nearby star (despite having a Gl number).
HU UMa| 57731| VB A (B = GSC 3014.0222 = L265-581, 24", 250 deg, common proper motion).
V0921 Cen| 57737| High proper motion (LTT 4397) not confirmed by HIPPARCOS data.
TY Crv| 58587| SB2.
KU Mus| 59665| Type RV: is also possible.
II UMa| 61237| Type RR: is also possible.
V0933 Cen| 61362| HIPPARCOS data contradict the luminosity class V.
DU Cru| 62918| The identification with NSV 06012 (SIMBAD) is wrong.
LV Vir| 66078| Type RR: is also possible.
CS CVn| 66682| HIPPARCOS data contradict the luminosity class V.
MW Vir| 69828| Type DSCTC: is also possible.
NN Vir| 70020| Type EW: is also possible.
V1015 Cen| 71967| Variability type and luminosity class (III) do not agree.
EL Boo| 72391| Type E: is also possible.
SZ UMi| 72625| Variability needs confirmation.
OU Ser| 75269| SB2.
gam Lup| 76297| SB, Porb = 2.8081d.
PS Ser| 77045| Both components are SB systems, Porb(A) = 15.888d, Porb(B) = 13.561d.
PT Ser| 77227| SB, Porb = 38.937d.
phi Her| 79101| SB, Porb = 560.5d.
V0367 Nor| 79490| May be not a supergiant.
V0374 Nor| 80557| Type LBV: is also possible.
V0946 Her| 84752| Not Wolf 688, a large-proper-motion star, which is at 17h19m28s.9, +33deg05'10" (epoch and equinox 2000.0).
V0973 Her| 88067| Suspected rapid brightness variations.
V2391 Oph| 88601| Porb = 88.13yr. Component B is a suspected variable star (NSV 24260) and may be the cause of variations.
V0870 Ara| 88853| Type DSCT: is also possible.
V4390 Sgr| 90001| SB2 and speckle binary.
V0994 Her| 90483| The secondary component of the double system may also vary.
V0531 Lyr| 90880| Minima observed only between JD 2448600 and 2448800.
QZ Tel| 91832| The variability may be due to the fainter (B) component.
V0550 Lyr| 93808| SB, Porb = 1.0309d.
V4417 Sgr| 95313| The variability may be due to the fainter (B) component.
V0337 Tel| 95578| Type EW: is also possible.
V0339 Sge| 96599| Extremely metal-weak.
V2105 Cyg| 98729| Variability type and spectral type (F8Iab:) do not agree.
V1470 Aql| 98826| The variability may be due to the fainter (B) component.
V1472 Aql| 98954| SB, Porb = 198d.
V4429 Sgr| 99042| A giant, according to HIPPARCOS data, despite the published luminosity class (V).
V0398 Vul| 99402| Not identical to IRC+30416 = NSV 12861.
V2121 Cyg|100859| Strong Blazhko effect.
BH Cap|100869| Type RR: is also possible.
V0382 Pav|101286| Type EW: is also possible.
alf Oct|104043| SB, Porb = 9.073d.
V0421 Cep|105091| SB, Porb1 = 5.4136d, Porb2 = 225.44d.
V2150 Cyg|105162| Type RR: is also possible.
BN Cap|105324| The variability may be due to the fainter (B) component.
V2174 Cyg|108476| SB, Porb = 225.162d.
V2175 Cyg|108738| X-ray source.
zet Cep|109492| Radial velocity varies.
V0447 Cep|109505| The variability may be due to the fainter (B) component.
V0448 Cep|109606| SB, Porb = 7.7320d.
KV Aqr|110707| One deep fading overlapping a brightening trend.
V0412 Lac|111022| SB, Porb = 41.95yr.
V0413 Lac|111071| SB, Porb = 2.9833d.
QQ Peg|111932| Variability needs confirmation.
V0453 Cep|112972| SB, Porb = 54.723d.
V0454 Cep|113065| SB, Porb = 5.6556d.
V0341 Peg|114024| SB, Porb = 2.1779d.
V0342 Peg|114189| Suspected SB.
CG Phe|116103| Type RRC: is also possible.
DX Tuc|118096| Type RRC: is also possible.