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Close-in stellar companions in close binary stars
Liao WP(廖文萍)1,2; Qian SB(钱声帮)1,2,3; Zhu LY(朱俐颖)1,2,3; Liu L(刘亮)1,2,3
会议录名称Publications of The Korean Astronomical Society
2015-09
卷号30
期号2
页码215-216
DOI10.5303/PKAS.2015.30.2.215
产权排序第1完成单位
收录类别其他
会议名称12th Asia-Pacific Regional IAU Meeting
会议日期2014-08-18
会议地点DOC, Daejeon, Korea
关键词Binaries: Close Binaries : Eclipsing Stars: InDividual (Di Hya V384 Ser V401 Cyg)
摘要
Close binary stars are so close that one component has an effect on the evolution of the other. But how do they form and evolve? This is an unsolved problem. One speculation is that the binary is a part of a hierarchical triple and its orbit shrinks due to interaction with the third component. Therefore, searching for and investigating tertiary components, especially close-in ones, in close binary stars are important for understanding their origin, as well as to test theories of star formation and stellar dynamical interaction.
语种英语
学科领域天文学
出版者The Korean Astronomical Society
出版地Korea
ISSN号1225-1534
URL查看原文
归档日期2016-05-10
引用统计
文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/9776
专题双星与变星研究组
中国科学院天体结构与演化重点实验室
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, P. R. China
2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences
3.University of Chinese Academy of Sciences, 100049, Beijing, P. R. China/Yuquan Road 19#, ShijingShan Block, 100049, Beijing City, P. R. China
推荐引用方式
GB/T 7714
Liao WP,Qian SB,Zhu LY,et al. Close-in stellar companions in close binary stars[C]. Korea:The Korean Astronomical Society,2015:215-216.
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