FOSSIL MAGNETIC FIELDS IN INTERMEDIATE-MASS AND MASSIVE STARS

被引：7
|
作者：
Alecian, E. [1 ]
Villebrun, F. [1 ]
Grunhut, J. [2 ]
Hussain, G. [3 ]
Neiner, C. [4 ]
Wade, G. A. [5 ]
机构：
[1] Univ Grenoble Alpes, CNRS, IPAG, F-38000 Grenoble, France
[2] Univ Toronto, Dunlap Inst Astron & Astrophys, Toronto, ON M5S 3H4, Canada
[3] European Southern Observ, D-85748 Garching, Germany
[4] UPMC Univ Paris 06, Univ Paris Diderot, Sorbonne Paris Cite, LESIA,Observ Paris,PSL Res Univ,CNRS,Sorbonne Uni, F-92195 Meudon, France
[5] Royal Mil Coll Canada, Dept Phys, Kingston, ON K7K 7B4, Canada
来源：
ASTRO FLUID 2016 | 2019年 / 82卷
基金：
加拿大自然科学与工程研究理事会;
关键词：
AP STARS; STELLAR EVOLUTION; MAIN-SEQUENCE; MIMES SURVEY; DISCOVERY; II; MAGNETOSPHERE; SEARCH; LINKS;
D O I：
10.1051/eas/1982030
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A small fraction of the population of intermediate-mass and massive stars host strong and stable magnetic fields organised on large scales. These fields are believed to be remnants of star formation. It is however not clear how such fossil fields have been shaped during their formation and subsequent evolution. We report recent and ongoing studies on the magnetic properties of pre-main sequence stars and main sequence binaries, allowing us to make progress in this field.
引用
收藏
页码：345 / 355
页数：11
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