Evolution of Intermediate Mass and Massive Binary Stars: Physics, Mass Loss, and Rotation

被引：0
作者：
Vanbeveren, D. [1 ]
Mennekens, N. [1 ]
机构：
[1] Vrije Univ Brussel, Astron & Astrophys Res Grp, Brussels, Belgium
来源：
B(E) PHENOMENON: FORTY YEARS OF STUDIES | 2017年 / 508卷
关键词：
O-TYPE STARS; PRESUPERNOVA EVOLUTION; CHEMICAL EVOLUTION; MERGER RATE; R-PROCESS; SUPERNOVAE; FREQUENCY; NUCLEOSYNTHESIS; VELOCITIES; RATES;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In the present review we discuss the past and present status of the interacting OB-type binary frequency. We critically examine the popular idea that Be-stars and supergiant sgB[e] stars are binary evolutionary products. The effects of rotation on stellar evolution in general, stellar population studies in particular, and the link with binaries will be evaluated. Finally a discussion is presented of massive double compact star binary mergers as possible major sites of chemical enrichment of r-process elements and as the origin of recent aLIGO GW events.
引用
收藏
页码：121 / 130
页数：10
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