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| Query : 2002MNRAS.336.1247S |
2002MNRAS.336.1247S - Mon. Not. R. Astron. Soc., 336, 1247-1255 (2002/November-2)
Short-period near-contact binary systems at the beginning of the overcontact phase.
SHENGBANG Q.
Abstract (from CDS):
Combined with the published data on the other systems of the same type, a possible statistical connection between orbital period P and its rate of decrease dP/d t is obtained: dP/d t =-5.3x10 –7xP + 1.3x10 –7 d yr –1. This correlation indicates that the smaller the orbital period P is, the smaller its rate of change dP/d t will be. The correlation found in this paper indicates that there may be a smooth transition from A- and F-type NCBs with period decreases to the A- and F-type overcontact binaries that have period increases, and in that sense one may postulate that the NCBs may be the progenitors of the A-type W UMa systems and will be oscillating around a marginal-contact state as predicted by thermal relaxation oscillation (TRO) theory.
Abstract Copyright: RAS
Journal keyword(s): binaries: close - stars: evolution - stars: mass-loss.
Simbad objects: 21
| Number of rows : 21 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | V* CN And | SB* | 00 20 30.5419967784 | +40 13 33.806776620 | 10.24 | 9.706 | 9.423 | 9.145 | F5V | 132 | 0 | |
| 2 | V* AG Phe | EB* | 00 26 54.9000348696 | -39 52 55.141301964 | 9.262 | 8.96 | A9V | 47 | 0 | |||
| 3 | V* RT Scl | SB* | 00 36 28.0901607240 | -25 40 22.933477128 | 10.63 | 10.31 | A5N+F3 | 68 | 0 | |||
| 4 | V* V473 Cas | EB* | 01 34 52.2529811760 | +56 39 09.401888232 | G2 | 44 | 0 | |||||
| 5 | V* BV Eri | SB* | 03 51 53.3421308952 | -10 31 49.473027048 | 8.69 | F2V | 70 | 0 | ||||
| 6 | V* RU Eri | SB* | 03 54 43.7743708272 | -14 56 06.649278720 | 9.86 | 9.39 | F3V | 48 | 0 | |||
| 7 | V* GR Tau | SB* | 04 01 03.2344925232 | +20 24 50.248533276 | 10.80 | 10.36 | 10.43 | A5V | 84 | 0 | ||
| 8 | V* AK CMi | SB* | 07 40 15.5947357968 | +03 57 09.429480828 | 10.97 | 10.73 | A-F | 60 | 0 | |||
| 9 | BD+04 1850A | EB* | 07 54 07.0681137528 | +03 39 20.339693028 | 10.60 | 10.25 | 10.07 | F0(N) | 66 | 0 | ||
| 10 | V* UU Lyn | SB* | 09 15 29.9170737408 | +42 42 09.201921264 | 12.00 | 11.57 | A4 | 61 | 0 | |||
| 11 | V* AV Hya | EB* | 09 35 02.5455460296 | +05 19 24.033656460 | 11.31 | 10.96 | 10.83 | A1 | 61 | 0 | ||
| 12 | V* BF Vir | SB* | 13 47 52.5954181752 | -00 35 40.700631948 | 10.27 | 10.2 | A1IV | 72 | 0 | |||
| 13 | V* VW Boo | SB* | 14 17 26.0324550672 | +12 34 03.446878260 | 11.33 | 10.55 | 10.054 | 9.777 | G5V | 117 | 0 | |
| 14 | V* FT Lup | SB* | 14 59 52.6999478616 | -42 58 59.102940900 | 10.27 | 9.82 | F0V | 67 | 0 | |||
| 15 | V* V1010 Oph | SB* | 16 49 27.6690355320 | -15 40 04.682052912 | 6.40 | 6.19 | A3V | 158 | 0 | |||
| 16 | V* TT Her | SB* | 16 54 22.9664980392 | +16 50 13.123555584 | 9.97 | 9.68 | A2V | 108 | 0 | |||
| 17 | V* V388 Cyg | SB* | 20 29 12.8831999088 | +31 23 11.995096848 | 9.82 | 9.59 | A0 | 60 | 0 | |||
| 18 | V* BO Peg | EB* | 21 31 17.8728099024 | +11 56 46.498943040 | 11.9 | 12.22 | A7IV-V | 50 | 0 | |||
| 19 | V* RS Ind | EB* | 21 36 49.7394154464 | -70 20 00.751186716 | 9.84 | 9.51 | F4 | 43 | 0 | |||
| 20 | V* BE Cep | EB* | 22 41 20.8003678104 | +58 36 31.133484036 | 12.94 | 12.05 | ~ | 49 | 0 | |||
| 21 | V* BL And | EB* | 23 11 24.2581546584 | +51 52 31.374661404 | 11.47 | 11.10 | A8 | 66 | 0 |
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