Main-sequence magnetic CP stars III. Results of magnetic field measurements

被引:7
作者
Romanyuk, I. I. [1 ]
机构
[1] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Russia
基金
俄罗斯基础研究基金会;
关键词
CHEMICALLY PECULIAR STARS; COOL AP-STAR; ABUNDANCE DISTRIBUTION GEOMETRY; RADIAL-VELOCITY VARIATIONS; STELLAR EVOLUTION; 53; CAMELOPARDALIS; AP/BP STARS; 78; VIRGINIS; B-STAR; SEARCH;
D O I
10.1134/S1990341310040048
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the third part of the survey of magnetic parameters of main-sequence magnetic CP stars. We analyze the main definitions and terminology, basic data on the magnetic fields of CP stars (catalogs, the history of the stellar magnetism research, the main observational results obtained over 60 years of studies). We describe the modern views on the properties of magnetic CP stars, i.e. their geometric structure, distribution of field strengths, magnetic field and rotation, magnetic field and energy distribution anomalies, and the evolutionary status of magnetic CP stars. We conclude that the observational data mostly support the theory of the relict origin and evolution of magnetic fields of CP stars.
引用
收藏
页码:347 / 380
页数:34
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