Mixing in stars

被引:270
作者
Pinsonneault, M
机构
[1] Astronomy Department, Ohio State University, Columbus, OH 43210
关键词
stellar evolution; stellar abundances; stellar rotation;
D O I
10.1146/annurev.astro.35.1.557
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Three cases for mixing not present in standard stellar models are presented: Light element depletion in low mass main-sequence stars, deep mixing in massive stars, and deep mixing in low mass giants. The review begins with the mixing indicators and the predictions of standard models. The observational evidence for anomalous mixing is then presented, followed by the physics of mixing outside the standard model. The status of theoretical models that include extra mixing is then examined.
引用
收藏
页码:557 / 605
页数:49
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