The Geneva stellar evolution code

被引：245

作者：

Eggenberger, P. ^{[1
]}

Meynet, G. ^{[1
]}

Maeder, A. ^{[1
]}

Hirschi, R. ^{[2
]}

Charbonnel, C. ^{[1
,3
]}

Talon, S. ^{[4
]}

Ekstroem, S. ^{[1
]}

机构：

[1] Univ Geneva, Observ Geneva, CH-1290 Sauverny, Switzerland

[2] Univ Basel, Dept Phys & Astron, CH-4052 Basel, Switzerland

[3] CNRS, UMR 5572, Lab Astrophys OMP, F-31400 Toulouse, France

[4] Univ Montreal, Dept Phys, Montreal, PQ H3C 3J7, Canada

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2008年 / 316卷 / 1-4期

基金：

英国科学技术设施理事会;

关键词：

stars; evolution;

D O I：

10.1007/s10509-007-9511-y

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This paper presents the Geneva stellar evolution code with special emphasis on the modeling of solar-type stars. The basic input physics used in the Geneva code as well as the modeling of atomic diffusion is first discussed. The physical description of rotation is then presented. Finally, the modeling of magnetic instabilities and transport of angular momentum by internal gravity waves is briefly summarized.

引用

收藏

页码：43 / 54

页数：12

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