Of?p stars: a class of slowly rotating magnetic massive stars

被引：2
|
作者：
Wade, Gregg A.
Grunhut, Jason H.
Marcolino, Wagner L. F.
Martins, Fabrice
Howarth, Ian D.
Naze, Yael
Walborn, Nolan R.
机构：
来源：
ACTIVE OB STARS: STRUCTURE, EVOLUTION, MASS-LOSS, AND CRITICAL LIMITS | 2011年 / 272期
关键词：
techniques: spectroscopic; stars: magnetic fields; stars:; individual; (HD; 191612; HD; 108; 148937); CLUES; FIELD;
D O I：
10.1017/S174392131101043X
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Only 5 Of?p stars have been identified in the Galaxy. Of these, 3 have been studied in detail, and within the past 5 years magnetic fields have been detected in each of them. The observed magnetic and spectral characteristics are indicative of organised magnetic fields, likely of fossil origin, confining their supersonic stellar winds into dense, structured magnetospheres. The systematic detection of magnetic fields in these stars strongly suggests that the Of?p stars represent a general class of magnetic O-type stars.
引用
收藏
页码：220 / 221
页数：2
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