3D anelastic simulations of convection in massive stars

被引：0
|
作者：
Kuhlen, M [1 ]
Wosley, SE [1 ]
Glatzmaier, GA [1 ]
机构：
[1] Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA
来源：
3D STELLAR EVOLUTION | 2003年 / 293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：
After briefly describing the anelastic approximation and Glatzmaier's code, we present results from our preliminary studies of core convection during the hydrogen burning phase of a 15Mcircle dot star, as well as our most recent results concerning convection in the oxygen shell of a 25Mcircle dot star.
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页码：147 / 156
页数：10
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