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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
Source PublicationAstronomical Society of the Pacific (ASP) Conference Series - TENTH PACIFIC RIM CONFERENCE ON STELLAR ASTROPHYSICS
2014-08
Volume482
Pages151-155
Author of SourceLee, HW; Leung, KC; Kang, YW
Contribution Rank第1完成单位
Indexed ByCPCI
Conference Name10th Pacific Rim Conference on Stellar Astrophysics
Conference Date2013-05-27
Conference PlaceSejong University Convention Center, Seoul, Korea
Abstract

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.

Funding ProjectChinese 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
Funding OrganizationChinese Natural Science Foundation ; West Light Foundation of the Chinese Academy of Sciences
Language英语
Subject Area天文学 ; 天体物理学
MOST Discipline Catalogue理学 ; 理学::天文学
SubtypeProceedings Paper
PublisherASTRONOMICAL SOC PACIFIC
Publication Place390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA
ISBN978-1-58381-849-7; 978-1-58381-848-0
URL查看原文
Archive Date2015-07-20
WOS IDWOS:000374279800026
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics ; Astronomy & Astrophysics
WOS KeywordVelocity Curves ; Light ; Parameters
Citation statistics
Document Type会议论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/9665
Collection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
Corresponding AuthorLiu L(刘亮)
Affiliation1.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
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Corresponding Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Liu L,Chen, Wenping,Qian SB,et al. Contact Binaries in the Galactic Star Cluster Berkeley 39[C]//Lee, HW; Leung, KC; Kang, YW. 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA:ASTRONOMICAL SOC PACIFIC,2014:151-155.
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