Massive star evolution

被引：0
|
作者：
Langer, N
Heger, A
机构：
[1] Univ Potsdam, Inst Phys, D-14415 Potsdam, Germany
[2] Max Planck Inst Astrophys, D-85740 Garching, Germany
来源：
NEW VIEWS OF THE MAGELLANIC CLOUDS | 1999年 / 190期
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The evolution of massive stars is far from being fully understood, as we outline by pointing to a number of open problems related to massive stars in the Magellanic Clouds. We argue that rotation may be a key ingredient in the physics of massive stars. We report on recent results obtained including rotation, and their relevance to these remaining questions.
引用
收藏
页码：192 / 199
页数：8
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