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
收藏
页码：345 / 348
页数：4
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