Radial velocity studies of close binary stars. II.

被引：85

作者：

Rucinski, SM ^{[1
]}

Lu, WX ^{[1
]}

机构：

[1] Univ Toronto, David Dunlap Observ, Richmond Hill, ON L4C 4Y6, Canada

来源：

ASTRONOMICAL JOURNAL | 1999年 / 118卷 / 05期

关键词：

binaries : close; binaries : eclipsing; stars : variables : general;

D O I：

10.1086/301101

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Radial velocity measurements and simple sine-curve fits to the orbital velocity variations are presented for the second set of 10 contact binary systems. Eight systems are of the A type: AH Aur, CK Boo, DK Cyg, UZ Lee, XZ Lee, V839 Oph, GR Vir, and NN Vir; V842 Her is the only W type, while SV Equ appears to be a semidetached system seen at a low orbital inclination rather than a contact binary. Several of the studied systems are prime candidates for complete light and radial velocity synthesis solutions.

引用

页码：2451 / 2459

页数：9

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