Mass loss from massive zero-metallicity stars

被引：0
|
作者：
Krticka, Jiri
Kubat, Jiri
机构：
[1] Masaryk Univ, CZ-61137 Brno, Czech Republic
[2] Astronom Ustav AV CR, CZ-25165 Ondrejov, Czech Republic
来源：
Stellar Evolution at Low Metallicity: Mass Loss, Explosions, Cosmology | 2006年 / 353卷
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：
We show that the radiative force is not able to drive a stellar wind from non-rotating hot massive zero-metallicity stars. This means that stellar winds from stationary massive hot first generation stars are unlikely. We study the possibility of expulsion of chemically homogeneous winds and the role of minor isotopes.
引用
收藏
页码：133 / 140
页数：8
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