ROTATION OF RED GIANTS

被引：0
作者：
Kissin, Y. [1 ,2 ]
Thompson, C. [2 ]
机构：
[1] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada
[2] Canadian Inst Theoret Astrophys, Toronto, ON M5H 3H8, Canada
来源：
PHYSICS OF EVOLVED STARS: A CONFERENCE DEDICATED TO THE MEMORY OF OLIVIER CHESNEAU | 2015年 / 71-72卷
关键词：
D O I：
10.1051/eas/1571075
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A new rotation model for post-main sequence stars is proposed. This model quantitatively reproduces core and surface rotation rates of subgiant stars, as well as the core rotation of helium-burning clump stars.
引用
收藏
页码：321 / 324
页数：4
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