Features of Magnetic Field Structures in Chemically Peculiar Stars. IV

被引：8

作者：

Glagolevskij, Yu. V. ^{[1
]}

Nazarenko, A. F. ^{[1
]}

机构：

[1] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Russia

来源：

ASTROPHYSICAL BULLETIN | 2016年 / 71卷 / 04期

关键词：

stars: magnetic field; stars: chemically peculiar; stars: evolution; HELIUM-STRONG STARS; THETA(1) ORIONIS-C; B-STARS; EVOLUTION FEATURES; WIND; AXES; SPECTROPOLARIMETRY; CONFINEMENT; ORIENTATION; VELOCITIES;

D O I：

10.1134/S1990341316040088

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present results of modeling of the sample of magnetic stars. We have obtained such important for magnetic star physics parameters as the mean surface magnetic field B-s, the magnetic field at magnetic poles-B-p, the dipole inclination to the rotation equatorial plane a, and the distance to monopoles from the center of the star Delta a. We present some information on magnetic star physics that helps to understand the derived results better.

引用

页码：453 / 462

页数：10

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