Protostellar collapse with various metallicities

被引：0
|
作者：
Omukai, K [1 ]
机构：
[1] Kyoto Univ, Dept Phys, Sakyo Ku, Kyoto 6068502, Japan
来源：
FIRST STARS | 2000年
关键词：
D O I：
10.1007/10719504_52
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The thermal and chemical evolution of gravitationally collapsing protostellar clouds are investigated focusing attention on their dependence on metallicity. The size of the stellar core at the formation is found to be the same regardless of the gas composition of the parent cloud.
引用
收藏
页码：277 / 278
页数：2
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