O-C Diagrams Analysis of Contact Binary Stars

被引：0
|
作者：
Liao, W-P. [1 ]
Qian, S-B. [1 ]
He, J-J. [1 ]
Zhu, L-Y. [1 ]
Liu, L. [1 ]
机构：
[1] Chinese Acad Sci, Yunnan Observ, POB 110, Kunming 650011, Peoples R China
来源：
TENTH PACIFIC RIM CONFERENCE ON STELLAR ASTROPHYSICS | 2014年 / 482卷
关键词：
CYCLIC PERIOD CHANGES; RADIAL-VELOCITY; ECLIPSING BINARIES; CLOSE BINARIES; RS CVN; COMPONENTS; VIRGINIS; ALGOL;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The variations of the orbital period of eclipsing stars can be derived by analyzing the (O - C) diagram. Combining our new CCD times of light minimum with the others published in the literature, the new orbital period analysis of some contact binary stars have been obtained by our group in recent years.
引用
收藏
页码：89 / 94
页数：6
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