A Model for Adiabatic Mass-loss

被引：1
|
作者：
Ge, Hongwei [1 ,3 ]
Webbink, R. F. [2 ]
Han, Z. [1 ]
机构：
[1] Chinese Acad Sci, Yunnan Observ, Natl Astron Observ, Kunming 650011, Yunnan, Peoples R China
[2] Univ Illinois, Dept Astron, Urbana, IL 61801 USA
[3] Chinese Acad Sci, Grad Univ, Beijing 100039, Peoples R China
来源：
ART OF MODELLING STARS IN THE 21ST CENTURY | 2008年 / 252期
基金：
美国国家科学基金会;
关键词：
stars: evolution; stars: interiors; stars: mass loss; binaries: close;
D O I：
10.1017/S1743921308023363
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
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.
引用
收藏
页码：419 / +
页数：2
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