Magnetic Fields in Low-Mass Stars: An Overview of Observational Biases

被引：0
|
作者：
Reiners, Ansgar [1 ]
机构：
[1] Georg August Univ Gottingen, Inst Astrophys, D-37077 Gottingen, Germany
来源：
MAGNETIC FIELDS THROUGHOUT STELLAR EVOLUTION | 2014年 / 302期
关键词：
ACTIVITY-ROTATION RELATIONSHIP;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Stellar magnetic dynamos are driven by rotation, rapidly rotating stars produce stronger magnetic fields than slowly rotating stars do. The Zeeman effect is the most important indicator of magnetic; fields, but Zeeman broadening must be disentangled from other broadening mechanisms, mainly rotation. The relations between rotation and magnetic field generation, between Doppler and Zeeman line broadening, and between rotation. stellar radius. and angular momentum evolution introduce several observational biases that affect our picture of stellar magnetism. In this overview, a few of these relations are explicitly shown, and the currently known distribution of field measurements is presented.
引用
收藏
页码：156 / 163
页数：8
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