Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.sai.msu.su/gcvs/gcvs/nl80/nl80_part_3/80_3rem.txt Дата изменения: Mon Mar 25 13:06:06 2013 Дата индексирования: Sat Mar 1 04:44:31 2014 Кодировка: Поисковые слова: релятивистское движение

V0499 Ser | Multiperiodic.
V0501 Ser | P = 0.266086d is also possible.
V0338 TrA | VB A (6.3mJ; B 10.3mJ, 7", 265deg, 2000).
V1327 Sco | VB (0.3", 5deg, 1995).
V1158 Her | Type RRC with a twice shorter period is possible.
CT CrB | Strong Blazhko effect.
V0479 Nor | Multiperiodic; P2 = 0.204945d.
V1331 Sco | In the region of the globular cluster M4. Cluster non-member.
V2683 Oph | Blazhko effect, P = 26.28d [377].
V2690 Oph | Porb = 0.063791d.
V0354 Dra | A magnetic white dwarf with unusual properties. Variations are probably related to spots and axial rotation.
V1211 Her | Multiperiodic.
V0898 Ara | Multiperiodic.
V0344 TrA | VB B (A = NEXT STAR IN THE LIST; AB 13", 304deg, 2000).
V0345 TrA | VB A (B = PREVIOUS STAR IN THE LIST, 13", 304deg, 2000).
V1364 Sco | Multiperiodic.
V1227 Her | Porb = 0.06319d.
V2703 Oph | VB A (B 14.3m, 19", 27deg, 1997).
V1231 Her | VB A (B 12.9mV, 12", 289deg, 1999).
V1236 Her | VB AB (10.2m, 11.2m, 1.3", 331deg, 2009).
V1414 Sco | OH maser.
V1239 Her | Eclipsing variability in quiescence: 17.4m - 19.1mV, Min = 2453648.236507 + 0.10008215d x E, D = 0.1P.
V2709 Oph | Blazhko effect, P = 22.18d.
V2711 Oph | Multiperiodic.
V2715 Oph | VB, a close companion to the north-west.
V1452 Sco | Multiperiodic.
V0363 Dra | Fundamental period: see Table. First overtone: P1 = 0.40320d.
V1250 Her | Ultraviolet flare amplitude in excess of 1.4m.
V1485 Sco | VB A (B 15.6m, 7", 244deg, 1999).
V1488 Sco | VB A (9.56mJ; B 9.74mJ, 6", 245deg, 1999).
V2718 Oph | Cluster non-member.
V2719 Oph | Cluster non-member. Type RRC a twice shorter period is not excluded.
V2720 Oph | Cluster non-member. Type EW with P=0.4225d is also possible.
V2721 Oph | Cluster non-member.
V0366 Dra | Multiperiodic, P = 0.0015926d is also excited.
V0368 Dra | Near the Draco dwarf galaxy; non-member.
V2724 Oph | O'Connell effect.
V0372 Dra | O'Connell effect.
V1504 Sco | The long period is about 735d.
V1506 Sco | VB A (B 14.04m, 10", 333deg, 2000; several other components. Second periodicity: P = 0.423350d or twice shorter.
V1265 Her | Blazhko effect?
V2731 Oph | Intermediate polar. Variations with Porb (see Table) and Pspin = 0.0014815d.
V1512 Sco | P2 = 0.058920d. VB AB (10.6, 11.0, 0".5, 204deg, 1991).
V2742 Oph | Biperiodic, P2 = 0.84443d.
V0909 Ara | Called "BH Ara?" in [80474]; the suggested identification is wrong.
V1285 Her | The elements tabulated are for the first overtone. P0 = 0.5539d.
V2744 Oph | The identification with NSV 09496 suggested in [80002] is wrong.
V1290 Her | SB1, Porb = 45.6228d.
V0381 Dra | The tabulated light elements are for eclipses. Oscillations with P = 0.04407d and amplitudes 0.04mR, 0.05mV, 0.07mB, also present at both minima.
V1517 Sco | Foreground star, globular cluster non-member.
V1299 Her | Type SRB is not excluded.
V1520 Sco | Foreground star, globular cluster non-member.
V1302 Her | VB B (A 12.2mV; B 12.4mV, 13", 266deg, 1998).
V1304 Her | VB A (B 12.1m, 16", 329deg, 2000).
V0386 Dra | VB B (A 13.5mF; B 14.0mF, 8", 16deg, 2000); the tabulated range is for combined brightness.
V0388 Dra | O'Connell effect.
V1314 Her | Blazhko effect?
V5627 Sgr | A decline from 15.1m to 16.9m was observed between JD 2449800 and 2451400. The tabulated light elements are for eclipses in quiescence (Max 16.88m).
V0737 CrA | Multiperiodic, P2 = 0.156795d.
V1323 Her | Intermediate polar; variations with only the spin period were detected. Porb = 0.11126d.
V5631 Sgr | VB A (B 11.2m, 1".9, 98deg, 2002).
V2770 Oph | A one-day alias, P = 0.10096d, is also possible.
V5632 Sgr | OH maser.
V0738 CrA | Globular cluster non-member?
V0739 CrA | Globular cluster non-member?
V0740 CrA | Globular cluster non-member?
V2775 Oph | O'Connell effect.
V0741 CrA | P = 0.394d is also possible. Globular cluster non-member?
V5633 Sgr | Multiperiodic.
V0742 CrA | Globular cluster non-member?
V0743 CrA | Globular cluster non-member?
V2780 Oph | The light curve shape varies.
V0745 CrA | Globular cluster non-member?
V2787 Oph | O'Connell effect.
V5634 Sgr | X-ray pulses with P = 5.539917s.
V5639 Sgr | VB A (B 11.6m, 8", 142deg, 2000; several fainter companions).
V0539 Ser | Multiperiodic.
V0641 Lyr | P = 0.4599d is not excluded.
V5640 Sgr | Erroneously called V1592 Sgr in [80502].
V5641 Sgr | Multiperiodic, P2 = 0.203290d.
V0498 Sct | Multiperiodic.
V1344 Her | MinII - MinI = 0.545P.
V2817 Oph | VB B (A 12.4m; AB 10", 34deg, 2000).
V0664 Lyr | VB A (A 13.0mV; B 14.5mV, 11", 302deg, 1998).
V5644 Sgr | The fundamental period is tabulated; for the first overtone, P = 0.34247d.
V0410 Dra | VB A (B 11.7mV, 8", 37deg, 2006).
V0374 Tel | The first-overtone period is tabulated; for the fundamental mode, P = 0.47907d.
V0413 Pav | P varies, dP/dt =+1.29 x 10^(-5) d/yr.
V0668 Lyr | Multiperiodic.
V0413 Dra | VB AB (A 7.4m var, SB; B 10.2m, 0.5", 34deg, 2008).
V0414 Dra | Type ELL with a twice longer period is also possible.
V1732 Aql | O'Connell effect.
V0416 Dra | Eclipses of about 0.2m in depth, Min = 2452368.53243 + 0.189109d x E.
V1737 Aql | VB A (B 12.2m, 7", 130deg, 2000).
V5649 Sgr | Blended, combined magnitudes are tabulated. Type Mira is not excluded.
V1742 Aql | VB A (B 16.5m, 2" sp).
V1743 Aql | The elements tabulated are for EB variations. EA: amplitude 0.14m, Min = 2450646.669 + 1.1920d, D = 0.14P.
V1752 Aql | P2 = 0.3586d.
V1760 Aql | P2 = 0.8381d.
V1801 Aql | A post-asymptotic-branch star. SB, Porb = 119.5d, e = 0.37. Porb is not detected in photometry.
V0691 Lyr | O'Connell effect.
V0722 Lyr | A post-asymptotic-branch star with non-periodic, sometimes rapid, brightness variations.
V0723 Lyr | Multiperiodic, P2 = 0.0745095d.
V2498 Cyg | Multiperiodic, P2 = 0.094d.
V2500 Cyg | Multiperiodic, P2 = 0.0677332d.
V0379 Tel | VB A (B 18.52m, 2.4").
V0469 Vul | Red, despite Sp B in the literature.
V0416 Pav | P0 is tabulated, P1 = 0.36574d.
V1811 Aql | A twice shorter period is not excluded.
AK UMi | Type ELL with a twice longer period is not excluded.
V0477 Vul | Multiperiodic, P2 = 0.0644149d.
V0479 Vul | Multiperiodic, P2 = 0.10114d.
V0425 Dra | MinII - MinI = 0.547:P.
V0378 Sge | VB A (B 13.7m, 20", 322deg, 2000).
V0491 Vul | MinII - MinI = 0.327P. VB AB (10.9m, 11.1m, 0.6", 223deg, 2010).
V0495 Vul | MinII - MinI = 0.544P.
V0380 Sge | VB AB (10.7m, 10.9m, 0.57", 74deg, 1990).
V0381 Tel | VB (11", 6deg, 2000); combined magnitudes are tabulated. For the first-overtone period, see the Table; P0 = 0.46781d; the amplitude ratio (1O/F) is 1.05.
V1815 Aql | A magnetic white dwarf, varies presumably due to starspots and axial rotation.
V2517 Cyg | VB A (B 14.1m, 5", 84deg, 1998).
V5659 Sgr | Blazhko effect, P = 45.69d.
V0498 Vul | Superhumps: P = 0.05990d. A possible cycle between outburtsts is about 1000d.
V0432 Dra | MinII - MinI = 0.698P.
V0810 Cep | O'Connell effect.
V1820 Aql | O'Connell effect.
V5664 Sgr | Type EW with a twice longer period is possible.
V0441 Dra | A twice shorter period is not excluded.
V2533 Cyg | Multiperiodic, P2 = 0.162486d, P3 = 0.148877d.
V2534 Cyg | Multiperiodic, P2 = 0.171077d, P3 = 0.239556d. VB A (B 12.0, 3", 165deg, 2003; C 12.5, 10", 112deg, 2003; D 13.1, 16", 2931deg, 2003).
V2536 Cyg | VB B (A 9.7m; AB 7", 270deg, 2003).
V2541 Cyg | A twice longer period is also possible.
V2544 Cyg | Apsidal motion detected. The tabulated elements are for MinI. MinII = 2455005.5824 + 2.093799d x E.
V2547 Cyg | SB.
V0818 Cep | Cluster non-member.
V0821 Cep | VB A (B 17.9mR, 4", 253deg, 2000).
V0822 Cep | Type EW with a twice longer period is not excluded [001].
V0507 Vul | Period varies. Light elements for JD 2454200-2455150 are tabulated. For JD 2452750-2453950, Max = JD 2453169.815 + 0.336042 x E.
V2566 Cyg | Multiperiodic, P2 = 0.422d. Porb = 55.03d.
QT Aqr | Porb = 0.074665d.
QU Aqr | Porb = 0.08330d.
V0835 Cep | Type RRC with the light elements Max = 2451511.899 + 0.2261d x E is not excluded.
V0839 Cep | VB AB (9.9m, 11.7m, 0.2", 212deg, 2008). MinII - MinI = 0.511P.
QV Aqr | VB A (B 19.1mg, 4", 228deg, 2001). Porb = 0.07196d.
QW Aqr | The first-overtone period is tabulated. P0 = 0.47722d, A1/A0 = 1.3.
V2581 Cyg | Multiperiodic. P2 = 0.2486d, P3 = 0.09029d.
V2583 Cyg | VB A (B 19.4m, 0.6", 0deg, 2002).
V2608 Cyg | Multiperiodic. P2 = 0.091463d.
VV Equ | Porb = 0.057083d.
V2618 Cyg | MinII - MinI = 0.57P.
V0429 Peg | Blazhko effect, P = 80.2d.
V2625 Cyg | VB A (B 5", 32deg, 1998).
CZ Ind | Blazhko effect, P = 133d.
V0850 Cep | MinII - MinI = 0.599:P.
V2642 Cyg | Total eclipses of the white dwarfs plus occasional small flares.
V2643 Cyg | O'Connell effect.
QZ Aqr | Superhumps: P = 0.064593d? [233].
DK Cap | Multiperiodic.
V0443 Peg | Blazhko effect from Catalina data [001].
V0444 Peg | Superhumps: P = 0.097762d [233].
V2647 Cyg | MinII - MinI = 0.334P.
V0460 Peg | The period of ellipsoidal variations is tabulated. Pulsational periods: 0.06479d and 0.06337d. The A8 component pulsates.
DM Cap | Porb = 0.2215d.
V0473 Peg | O'Connell effect.
V0479 Peg | Period varies.
V0492 Peg | P = 0.11068d for the main DSCTC mode. Multiperiodic, several other GDOR and DSCTC periods.
V0499 Peg | VB A (A 10.90mJ; B 11.50mJ, 9", 324deg, 2000).
V0873 Cep | Multiperiodic.
V0874 Cep | Multiperiodic.
V0510 Peg | Multiperiodic.
AE PsA | Blazhko effect, P = 5.78d.
V0513 Peg | Porb = 0.17918d.
V0517 Peg | Blazhko effect?
V0521 Peg | Porb = 0.05986d.
V0880 Cep | MinII - MinI = 0.540P.
V0881 Cep | MinII - MinI = 0.476:P.
V0882 Cep | VB A (B 14.6m, 7", 274deg, 1999).
V0533 Peg | VB AB (A 9.7mJ; B 11.3mJ, 4", 1 deg, 1998).
V0468 Lac | Multiperiodic.
EP Tuc | Blazhko effect, P = 63d.
V0897 Cep | MinII - MinI = 0.518P.
V0898 Cep | MinII - MinI = 0.670P.
V0349 Aqr | Pspin is tabulated. Porb = 0.1344d.
V0537 Peg | Porb = 0.42234d.
V0354 Aqr | Blazhko effect, P = 181.20d.
V0550 Peg | Blazhko effect.
V0553 Peg | Blazhko effect?
V0919 Cep | MinII - MinI = 0.44P.
V0921 Cep | MinII - MinI = 0.429P.
V0922 Cep | MinII - MinI = 0.585P. VB A (A 10.6mJ; B 11.9mJ, 11", 44deg; C 13.6mJ, 4", 76deg, 1999). Tabulated magnitudes are influenced with the companions.
V1183 Cas | Multiperiodic.
AG PsA | The first-overtone period is tabulated. P0 = 0.49785d. A1/A0 = 1.6.
V0604 And | The coordinates in [598] are wrong.
V0585 Peg | Multiperiodic.
EN Gru | P varies. dP/dt = +0.55 x 10^(-5) d/yr.
V0357 Aqr | P varies. dP/dt = -0.37 x 10^(-5) d/yr.
V0358 Aqr | Epoch of minimum is tabulated. High states: 15.7 - 16.8m; low states: 16.5 - 17.5m.
V0360 Aqr | Blazhko effect, P = 54.52d.
V0362 Aqr | Light elements for eclipses are tabulated. DSCTC: P = 0.038213d, Delta m = 0.03m.
V0944 Cep | MinII - MinI = 0.528P.
V0598 Peg | Porb is tabulated. Pspin = 0.02893d.
IN Psc | VB A (B 8", 48deg, 1999). Combined magnitudes are tabulated.
V0954 Cep | O'Connell effect.
V1194 Cas | Multiperiodic.
CX Scl | Light elements for eclipses are tabulated. DSCTC pulsations: P = 0.183038d, Delta m = 0.11m.
V0957 Cep | MinII - MinI = 0.560P.
V0615 Peg | Porb = 0.240946d from spectroscopy.
V0961 Cep | MinII-MinI=0.482P.
V1236 Cas | O'Connell effect.