Evolutionary Processes in Low-Mass Binary Systems

被引：0
作者：
Peter P. Eggleton
Ludmila Kisseleva-Eggleton
机构：
[1] Lawrence Livermore National Laboratory,Department of Mathematics
[2] University of the Pacific,undefined
来源：
Astrophysics and Space Science | 2005年 / 296卷
关键词：
double stars; dynamo activity; winds; magnetic braking; tidal friction;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
We consider the evolution of certain low-mass binaries, incorporating models of (a) internal evolution, (b) tidal friction, (c) dynamo activity driven by an elementary α,Ω dynamo, (d) stellar wind driven by the activity, and (e) magnetic braking as a consequence of wind and poloidal dynamo-generated magnetic field. In some circumstances the stellar wind is found to remove mass on a nuclear timescale, as is necessary to explain some observed systems.
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页码：327 / 336
页数：9
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