Angular Momentum Evolution of Young Solar-type Stars

被引：0

作者：

Amard, Louis ^{[1
,2
]}

Palacios, Ana ^{[1
]}

Charbonnel, Corinne ^{[2
,3
]}

机构：

[1] Univ Montpellier, LUPM, CNRS, Pl Eugene Bataillon, F-34095 Montpellier, France

[2] Univ Geneva, Geneva Observ, Chemin Maillettes 51, CH-1290 Versoix, Switzerland

[3] Univ Toulouse, IRAP Dept Astron, CNRS, UMR 5277, 14 Av E Belin, F-31400 Toulouse, France

来源：

YOUNG STARS & PLANETS NEAR THE SUN | 2016年 / 10卷 / 314期

关键词：

stars: evolution; stars: rotation; stars: wind-braking; hydrodynamics; STELLAR EVOLUTION; ROTATING STARS; CIRCULATION; TURBULENCE;

D O I：

10.1017/S174392131500647X

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present stellar evolution models of young solar-type stars including self consistent treatment of rotational mixing and extraction of angular momentum (AM) by magnetized wind including the most up-to-date physic of AM transport.

引用

页码：109 / 112

页数：4

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