On the coupled influence of rotation and magnetism in convective core of A-type stars

被引：0

作者：

Brun, AS ^{[1
]}

机构：

[1] CEA Saclay, DAPNIA, SAp, UMR AIM & DSM, F-91191 Gif Sur Yvette, France

来源：

Element Stratification in Stars: 40 Years of Atomic Diffusion: MEETING IN HONOUR OF GEORGES MICHAUD | 2005年 / 17卷

关键词：

D O I：

10.1051/eas:2005115

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We briefly report on an ongoing numerical project that aims at simulating, with the ASH code, the intricate magnetohydrodynamic processes present in the inner region of A-type stars. We mainly focus our attention, on the dynamics of the convective core, its associated differential rotation and meridional ciculation and the dynamo action than can occur in such tubulent MHD system. We indeed find that; magnetic fields with amplitude greater than 10 kG are likely to be present in the core of A-type stars.

引用

页码：203 / 208

页数：6

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