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The criteria for dynamical mass transfer of the main-sequence donor stars
Ge HW(葛宏伟)1,2; R. F. Webbink3; Chen XF(陈雪飞)1,2; Han ZW(韩占文)1,2
Source PublicationProceedings IAU Symposium - Feeding Compact Objects: Accretion on All Scales
2013-02
Volume290
Pages213-214
DOI10.1017/S1743921312019679
Contribution Rank第1完成单位
Indexed By其他
Conference Name290th IAU Symposium - Feeding Compact Objects: Accretion on All Scales
Conference Date2012-08-20
Conference PlaceBeijing, China
KeywordBinaries:Close Stars:Evolution Stars:Mass-loss Stars:Interios
Abstract

Mass transfer is very common in binary evolution and it dominates the evolutionary fate of binaries. Two crucial problems i.e. dynamical mass transfer and common envelope evolution, are not well understood yet. Here we focus on the first problem, and systematically show the critical mass ratio for dynamical mass transfer when the donor stars are still on the main sequence (MS).

Funding ProjectN/A
Funding OrganizationN/A
Language英语
Subject Area天文学 ; 天体物理学 ; 恒星与银河系
MOST Discipline Catalogue理学 ; 理学::天文学
URL查看原文
Archive Date2014-11-07
Citation statistics
Document Type会议论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/9652
Collection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
Affiliation1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China
2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming 650011, China
3.Department of Astronomy, University of Illinois, 1002 W. Green St. Urbana, IL 61801, USA
First Author AffilicationYunnan Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Ge HW,R. F. Webbink,Chen XF,et al. The criteria for dynamical mass transfer of the main-sequence donor stars[C],2013:213-214.
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