中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
THE FIRST PHOTOMETRIC ANALYSIS OF THE OVERCONTACT BINARY MQ UMa WITH AN ADDITIONAL COMPONENT

文献类型:期刊论文

作者Zhou X(周肖)1,2,3; Qian SB(钱声帮)1,2,3; Liao WP(廖文萍)1,2; Zhao EG(赵二刚)1,2,3; Wang JJ(王晶晶)1,2,3; Jiang LQ(江林巧)1,2,3
刊名ASTRONOMICAL JOURNAL
出版日期2015-09
卷号150期号:3
ISSN号0004-6256
产权排序第一完成单位
通讯作者Zhou, X (reprint author), Chinese Acad Sci, Yunnan Observ, POB 110, Kunming 650216, Peoples R China.
英文摘要The first V R-c I-c band light curves of MQ UMa are presented and analyzed using the Wilson-Devinney (W-D) program. It is discovered that MQ UMa is an A-subtype contact binary with a high fill-out (f = 82%) and a low mass ratio (q = 0.195), which indicates that it is in the late evolutionary stage of late-type tidal-locked binary stars. The mass of the primary and secondary stars is estimated and the evolutionary status of the two components are placed on the H-R diagram. The W-D solutions also indicate that MQ UMa may be a triple system with an additional F5V type component. A sample of 16 high fill-out, low mass ratio overcontact binaries is collected and their possible evolution scenarios are discussed. Using the five times of minimum light recently observed together with those collected from the literature, the authors find that the observed-calculated (O-C) curve exhibits cyclic period variation. The cyclic period change also reveals the presence of a tertiary component, which may play an important role in the formation and evolution of this binary system by drawing angular momentum from the central system.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]STAR LIGHT CURVES ; HIGH FILL-OUT ; VELOCITY CURVES ; DEEP ; CONTACT ; SYSTEMS ; PARAMETERS ; COMPANION ; BOOTIS ; CYGNI
收录类别SCI
原文出处http://iopscience.iop.org/1538-3881/150/3/83/
语种英语
WOS记录号WOS:000364008100020
源URL[http://ir.ynao.ac.cn/handle/114a53/5914]  
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
作者单位1.Yunnan Observatories, Chinese Academy of Sciences (CAS), P.O. Box 110, 650216 Kunming, China
2.Key Laboratory of the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, P.O. Box 110, 650216 Kunming, China
3.University of the Chinese Academy of Science, Yuquan Road 19#, Sijingshang Block, 100049 Beijing, China
推荐引用方式
GB/T 7714
Zhou X,Qian SB,Liao WP,et al. THE FIRST PHOTOMETRIC ANALYSIS OF THE OVERCONTACT BINARY MQ UMa WITH AN ADDITIONAL COMPONENT[J]. ASTRONOMICAL JOURNAL,2015,150(3).
APA Zhou X,Qian SB,Liao WP,Zhao EG,Wang JJ,&Jiang LQ.(2015).THE FIRST PHOTOMETRIC ANALYSIS OF THE OVERCONTACT BINARY MQ UMa WITH AN ADDITIONAL COMPONENT.ASTRONOMICAL JOURNAL,150(3).
MLA Zhou X,et al."THE FIRST PHOTOMETRIC ANALYSIS OF THE OVERCONTACT BINARY MQ UMa WITH AN ADDITIONAL COMPONENT".ASTRONOMICAL JOURNAL 150.3(2015).

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来源:云南天文台

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