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New Progress on High Fill-Out, Extreme Mass Ratio Overcontact Binary Systems
He JJ(何家佳)1,2; Qian SB(钱声帮)1,2; Soonthornthum, B3
会议录名称Astronomical Society of the Pacific (ASP) Conference Series - NINTH PACIFIC RIM CONFERENCE ON STELLAR ASTROPHYSICS
2012
卷号451
页码45-50
会议录编者/会议主办者Qian, SB; Leung, KC; Zhu, L; Kwok, S
产权排序第1完成单位
收录类别CPCI
会议名称9th Pacific Rim Conference on Stellar Astrophysics
会议日期2011-04-14
会议地点Lijiang, PEOPLES R CHINA
摘要

High Fill-Out, Extreme Mass Ratio Overcontact Binary (HFEMOB) are a very important source to understand the structure and evolution of the late-type short-period close binary stars, because they are at the late evolutionary stage of these systems. Recently, the detail photometric studies of fifteen such HFEMOBs, including GR Vir, IK Per, FG Hya, TV Mus, CU Tau, V857 Her, GSC619-232, V410 Aur, XY Boo, AH Cnc, QX and, EM Psc, V345 Gem, XY LMi and V 1191 Cyg were published. In the present paper, we summarize these results and give some new observations of some HFEMOB candidates.

语种英语
学科领域天文学 ; 天体物理学 ; 恒星与银河系
学科门类理学 ; 理学::天文学
文章类型Proceedings Paper
出版者ASTRONOMICAL SOC PACIFIC
出版地390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA
ISBN号978-1-58381-785-8
URL查看原文
归档日期2012-12-19
WOS记录号WOS:000304126300007
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]Deep ; Cygni
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被引频次:1[WOS]   [WOS记录]     [WOS相关记录]
文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/5951
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
通讯作者He JJ(何家佳)
作者单位1.National Astronomical Observatories/Yunnan Astronomical Observatory, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, China
2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 650011 Kunming, China
3.National Astronomical Research Institute of Thailand/Ministry of Science and Technology, Bangkok, Thailand
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He JJ,Qian SB,Soonthornthum, B. New Progress on High Fill-Out, Extreme Mass Ratio Overcontact Binary Systems[C]//Qian, SB; Leung, KC; Zhu, L; Kwok, S. 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA:ASTRONOMICAL SOC PACIFIC,2012:45-50.
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