Stellar adiabatic mass loss model and applications

doi:10.1007/s10509-010-0286-1

YNAO OpenIR > 大样本恒星演化研究组

	Stellar adiabatic mass loss model and applications
	Ge HW(葛宏伟)1,2,3 ; Webbink, RF 4; Han ZW(韩占文)1,2 ; Chen XF(陈雪飞)1,2 ; Ge, HW (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China.
发表期刊	ASTROPHYSICS AND SPACE SCIENCE
	2010-10
卷号	329 期号:1-2 页码:243-248
DOI	10.1007/s10509-010-0286-1
产权排序	第1完成单位
收录类别	SCI
关键词	Stars: Evolution Stars: Interiors Stars: Mass Loss Binaries: Close
摘要	Roche-lobe overflow and common envelope evolution are very important in binary evolution, which is believed to be the main evolutionary channel to hot subdwarf stars. The details of these processes are difficult to model, but adiabatic expansion provides an excellent approximation to the structure of a donor star undergoing dynamical time scale mass transfer. We can use this model to study the responses of stars of various masses and evolutionary stages as potential donor stars, with the urgent goal of obtaining more accurate stability criteria for dynamical mass transfer in binary population synthesis studies. As examples, we describe here several models with the initial masses equal to 1 M (aS (TM)) and 10 M (aS (TM)), and identify potential limitations to the use of our results for giant-branch stars.
项目资助者	National Natural Science Foundation of China [10821061, 10973036, 2007CB815406] ; U.S. National Science Foundation [AST 0406726] ; Chinese Academy of Sciences [KJCX2-YW-T24] ; Yunnan Natural Science Foundation [08YJ041001]
语种	英语
学科领域	Astronomy & Astrophysics
文章类型	Article
ISSN	0004-640X
URL	查看原文
归档日期	2010-10-13
WOS记录号	WOS:000282823200039
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	SUBDWARF-B-STARS ; BRANCH STARS ; EVOLUTION ; ORIGIN
引用统计	被引频次：14[WOS] [WOS记录] [WOS相关记录]
文献类型	期刊论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/4488
专题	大样本恒星演化研究组中国科学院天体结构与演化重点实验室
通讯作者	Ge, HW (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China.
作者单位	1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, P.R. China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, 650011, P.R. China 3.Graduate University of Chinese Academy of Sciences, Beijing, 100049, P.R. China 4.Department of Astronomy, University of Illinois, 1002 W. Green St., Urbana, IL, 61801, USA
第一作者单位	中国科学院云南天文台
推荐引用方式 GB/T 7714	Ge HW,Webbink, RF,Han ZW,et al. Stellar adiabatic mass loss model and applications[J]. ASTROPHYSICS AND SPACE SCIENCE,2010,329(1-2):243-248.
APA	Ge HW,Webbink, RF,Han ZW,Chen XF,&Ge, HW .(2010).Stellar adiabatic mass loss model and applications.ASTROPHYSICS AND SPACE SCIENCE,329(1-2),243-248.
MLA	Ge HW,et al."Stellar adiabatic mass loss model and applications".ASTROPHYSICS AND SPACE SCIENCE 329.1-2(2010):243-248.

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