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

页码：220 / 221

页数：2

共 50 条

[41] Rotating massive stars: From first stars to gamma ray bursts
Maeder, Andre
Meynet, Georges
REVIEWS OF MODERN PHYSICS, 2012, 84 (01) : 25 - 63
[42] Tidally driven mean flows in slowly and uniformly rotating massive main-sequence stars
Lee, Umin
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2017, 468 (02) : 1864 - 1880
[43] Nucleosynthesis in early rotating massive stars and chemical composition of CEMP stars
Choplin, A.
Hirschi, R.
NUCLEAR PHYSICS IN ASTROPHYSICS IX (NPA-IX), 2020, 1668
[44] SLOWLY ROTATING RELATIVISTIC STARS .9. MOMENTS OF INERTIA OF ROTATIONALLY DISTORTED STARS
HARTLE, JB
ASTROPHYSICS AND SPACE SCIENCE, 1973, 24 (02) : 385 - 405
[45] Evolution equations for the perturbations of slowly rotating relativistic stars
Ruoff, J
Stavridis, A
Kokkotas, KD
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2002, 332 (03) : 676 - 688
[46] Nonradial oscillations of slowly and differentially rotating compact stars
Stavridis, Adamantios
Passamonti, Andrea
Kokkotas, Kostas
PHYSICAL REVIEW D, 2007, 75 (06):
[47] Slowly rotating neutron stars in scalar torsion theory
Boumaza, Hamza
EUROPEAN PHYSICAL JOURNAL C, 2021, 81 (05):
[48] MODELS OF ROTATING MAGNETIC STARS
MESTEL, L
MOSS, DL
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1977, 178 (01) : 27 - 49
[49] Accuracy of the relativistic Cowling approximation in slowly rotating stars
Mon Not Royal Astron Soc, 1 (117):
[50] Magnetic fields of massive stars
Hubrig, Swetlana
Cure, Michel
Ilyin, Ilya
Schoeller, Markus
ACTIVE OB STARS: STRUCTURE, EVOLUTION, MASS-LOSS, AND CRITICAL LIMITS, 2011, (272): : 196 - +

← 1 2 3 4 5 →