On magnetic braking of late-type stars
On magnetic braking of late-type stars
复制标题
DOI：
10.1093/mnras/226.1.57
复制
发表时间：
1987-05
影响因子：
4.8
通讯作者：
L. Mestel;H. Spruit
中科院分区：
文献类型：
--
作者：
L. Mestel;H. Spruit
这份报告涉及晚型恒星到达主序星之后的自转历史。与本次研讨会相关的问题是，将磁制动理论与年轻星团的观测进行详细比较，是否会对发电机活动产生任何约束，特别是对表面场强B s与角速度Ω之间的关系。
This report deals with the rotational history of late-type stars subsequent to their reaching the main sequence. The question of relevance to this Symposium is whether detailed comparison of magnetic braking theory with observations of young stellar clusters will yield any constraints on dynamo activity, in particular on the relation between the surface field strength B s and the angular velocity Ω.