The energy transfer in W UMa binary stars

doi:10.1017/S1743921308023430

YNAO OpenIR > 大样本恒星演化研究组

	The energy transfer in W UMa binary stars
	Jiang DK(姜登凯)1,2 ; Wang JC(王建成)1 ; Han ZW(韩占文)1 ; Jiang TY(姜天雨)1,2 ; Li LF(李立芳)1
会议录名称	IAU Symposium Proceedings Series - ART OF MODELLING STARS IN THE 21ST CENTURY
	2008
卷号	4
期号	252
页码	433-434
DOI	10.1017/S1743921308023430
会议录编者/会议主办者	Deng, L; Chan, KL
产权排序	第1完成单位
收录类别	CPCI
会议名称	252nd Symposium of the International-Astronomical-Union
会议日期	2008-04-06
会议地点	Sanya, PEOPLES R CHINA
会议赞助商	Int Astron Union; Natl Nat Sci Fdn China; Chinese Acad Sci; Natl Astron Observatories
关键词	Stars: Evolution (Stars:) Binaries: Close (Stars:) Binaries: General
摘要	The properties of W UMa binary stars are studied based on the well-determined physical parameters of 132 W UMa systems. It is found that the energy transfer rate has a maximum value at q similar to 0.58. The relation between the energy transfer rate and the temperature deviation is also investigated, and the temperature of the secondary component is related to the energy transfer rate.
项目资助者	N/A
语种	英语
学科领域	天文学 ; 天体物理学 ; 恒星与银河系
文章类型	Proceedings Paper
出版者	CAMBRIDGE UNIV PRESS
出版地	THE PITT BUILDING, TRUMPINGTON ST, CAMBRIDGE CB2 1RP, CAMBS, ENGLAND
ISBN号	978-0-521-88983-4
ISSN号	1743-9213
URL	查看原文
归档日期	2008-11-06
WOS记录号	WOS:000263138600086
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	Contact Binaries
引用统计
文献类型	会议论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/243
专题	大样本恒星演化研究组
通讯作者	Jiang DK(姜登凯)
作者单位	1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China 2.Graduate University of Chinese Academy Sciences, Beijing 100039, China
第一作者单位	中国科学院云南天文台
通讯作者单位	中国科学院云南天文台
推荐引用方式 GB/T 7714	Jiang DK,Wang JC,Han ZW,et al. The energy transfer in W UMa binary stars[C]//Deng, L; Chan, KL. THE PITT BUILDING, TRUMPINGTON ST, CAMBRIDGE CB2 1RP, CAMBS, ENGLAND:CAMBRIDGE UNIV PRESS,2008:433-434.

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