A Model for Adiabatic Mass-loss
Ge HW(葛宏伟); Webbink, R. F.; Han ZW(韩占文); Ge HW(葛宏伟); Han ZW(韩占文)
2008
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
关键词stars: evolution stars: interiors stars: mass loss binaries: close
卷号4
期号252
页码419-420
通讯作者Ge, HW (reprint author), Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Peoples R China.
英文摘要We describe our work on the development and application of a stellar structure code to compute model sequences representing donor stars in interacting binaries subject to rapid (adiabatic) mass-loss. The donor star is assumed to remain in hydrostatic equilibrium, but no heat flow is allowed. These sequences can be used to define bifurcation sequences in close binary evolution, and to circumscribe possible survivors of common envelope evolution.
收录类别CPCI
产权排序第一完成单位
会议网址http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=2452128&fileId=S1743921308023363
会议录IAU Symposium Proceedings Series - ART OF MODELLING STARS IN THE 21ST CENTURY
会议录出版者CAMBRIDGE UNIV PRESS
会议录出版地THE PITT BUILDING, TRUMPINGTON ST, CAMBRIDGE CB2 1RP, CAMBS, ENGLAND
学科主题Astronomy & Astrophysics
语种英语
ISSN号1743-9213
ISBN号978-0-521-88983-4
内容类型会议论文
源URL[http://ir.ynao.ac.cn/handle/114a53/241]  
专题云南天文台_大样本恒星演化研究组
通讯作者Ge HW(葛宏伟)
推荐引用方式
GB/T 7714
Ge HW,Webbink, R. F.,Han ZW,et al. A Model for Adiabatic Mass-loss[C]. 见:252nd Symposium of the International-Astronomical-Union. Sanya, PEOPLES R CHINA. 2008-04-06.http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=2452128&fileId=S1743921308023363.
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