2002MNRAS.336.1247S


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):

A detailed analysis of orbital period changes of seven near-contact binary stars (NCBs) (BL And, V473 Cas, XZ CMi, BV Eri, RU Eri, UU Lyn and GR Tau) with period less than 1 d has been performed and their respective O-C diagrams are formed and discussed. It is found that all systems analysed show secular period decreasing. For V473 Cas, the analysis of the period change was performed based on data collected by Moschner, Frank & Bastian. For XZ CMi, its period shows some complex changes, a possible cyclic oscillation is discovered to superpose on the secular decrease that can be explained either by the presence of a third body or by magnetic activity cycles of the components. Since the third-body assumption is consistent with the photometric solution of Rafert, XZ CMi may be a truly triple system. For BV Eri, the period decrease is only supported by weak evidence. All the seven systems are short-period NCBs with AF-type primary components where both components are filling or nearly filling the critical Roche lobe. As the period decreases, the separation between both components will be reducing and thus these systems will evolve into A-type overcontact binaries. The period decrease may be caused by mass transfer or/and by angular momentum loss via magnetic braking.

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

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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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