The evolution of the internal rotation of solar-type stars

被引：0

作者：

Di Mauro, Maria Pia ^{[1
]}

Ventura, Rita ^{[2
]}

Cardini, Daniela ^{[1
]}

Christensen-Dalsgaard, Jorgen ^{[3
]}

Dziembowski, Wojciech A. ^{[4
]}

Paterno, Lucio

机构：

[1] INAF, IAPS Ist Astrofis & Planetol Spaziali, Via Fosso Cavaliere 100, I-00133 Rome, Italy

[2] INAF, Astrophys Observ Catania, I-95020 Catania, Italy

[3] Aarhus Univ, Dept Phys & Astron, Stellar Astrophys Ctr, DK-8000 Aarhus C, Denmark

[4] Univ Warsaw Observ, PL-00478 Warsaw, Poland

来源：

PRECISION ASTEROSEISMOLOGY | 2014年 / 9卷 / 301期

关键词：

stars: oscillations; stars: rotation; stars: evolution; Sun: helioseismology; Sun: evolution; Sun: rotation;

D O I：

10.1017/S1743921313014567

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We discuss the potential of asteroseismic inversion to study the internal dynamics of solar-type stars and to reconstruct the evolution of the internal rotation from the main sequence to the red-giant phase. In particular, we consider the use of gravity and mixed modes and the application of different inversion methods.

引用

页码：345 / 348

页数：4

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