Stars with a Stable Magnetic Field

被引：0
|
作者：
Ferrario, L. [1 ]
机构：
[1] Australian Natl Univ, Math Sci Inst, Canberra, ACT 2601, Australia
来源：
CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO | 2018年 / 48卷 / 01期
关键词：
stars: magnetic field; stars: protostars; stars: chemically peculiar; white dwarfs; pulsars; stars: magnetars; CHEMICALLY PECULIAR STARS; HERBIG AE/BE STARS; RESOLUTION SPECTROPOLARIMETRIC SURVEY; LARGE-MAGELLANIC-CLOUD; A-TYPE STARS; WHITE-DWARFS; NEUTRON-STARS; MAIN-SEQUENCE; X-RAY; STELLAR EVOLUTION;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this review I will summarise what we know about magnetic fields in stars and what the origin of these magnetic fields may be. I will address the issue of whether the magnetic flux is conserved from pre-main sequence to the compact star phase (fossil field origin) or whether fields may be dynamo generated during some stages of stellar evolution or perhaps during stellar merging events.
引用
收藏
页码：15 / 31
页数：17
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