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Contact Binaries in the Galactic Star Cluster Berkeley 39
Liu L(刘亮)1,2,3; Chen, Wenping4,5; Qian SB(钱声帮)1,2,3; Zhu LY(朱俐颖)1,2,3; He JJ(何家佳)1,2,3; Liao WP(廖文萍)1,2,3; Panwar, Neelam6
2014-08
会议日期2013-05-27
会议地点Sejong University Convention Center, Seoul, Korea
卷号482
页码151-155
英文摘要

The RI light curves of V6, V7 and V10 in the field of open cluster Be39 are presented and analyzed by the 2010 W-D code. The masses and radii of each component are estimated. V7 and V10 should be members of Be39 while V6 may be not a member.

源文献作者Lee, HW; Leung, KC; Kang, YW
产权排序第1完成单位
会议录Astronomical Society of the Pacific (ASP) Conference Series - TENTH PACIFIC RIM CONFERENCE ON STELLAR ASTROPHYSICS
资助机构Chinese Natural Science Foundation ; West Light Foundation of the Chinese Academy of Sciences
会议录出版者ASTRONOMICAL SOC PACIFIC
会议录出版地390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA
文献子类Proceedings Paper
学科主题天文学 ; 天体物理学
语种英语
URL标识查看原文
资助项目Chinese Natural Science Foundation[11103074] ; Chinese Natural Science Foundation[11133007] ; Chinese Natural Science Foundation[10973037] ; Chinese Natural Science Foundation[11203066] ; Chinese Natural Science Foundation[10903026] ; West Light Foundation of the Chinese Academy of Sciences
ISBN号978-1-58381-849-7; 978-1-58381-848-0
WOS研究方向Astronomy & Astrophysics
WOS记录号WOS:000374279800026
WOS关键词Velocity Curves ; Light ; Parameters
内容类型会议论文
源URL[http://ir.ynao.ac.cn/handle/114a53/9665]  
专题云南天文台_双星与变星研究组
云南天文台_中国科学院天体结构与演化重点实验室
通讯作者Liu L(刘亮)
作者单位1.Yunnan Observatory, 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, P.O. Box 110, 650011 Kunming, P. R. China
3.Graduate University of the Chinese Academy of Sciences, 19A Yuquanlu, Sijingshang Block, 100049 Beijing, China
4.Graduate Institute of Astronomy, National Central University, Taiwan
5.Dept of Physics, National Central University, Taiwan
6.Tenagra Observatory, Arizona, USA
推荐引用方式
GB/T 7714
Liu L,Chen, Wenping,Qian SB,et al. Contact Binaries in the Galactic Star Cluster Berkeley 39[C]. 见:. Sejong University Convention Center, Seoul, Korea. 2013-05-27.
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