On Properties of Main Sequence Magnetic Stars

被引：0
作者：
Yu. V. Glagolevskij
机构：
[1] Russian Academy of Sciences,Special Astrophysical Observatory
来源：
Astrophysical Bulletin | 2019年 / 74卷
关键词：
stars: magnetic fields; stars: chemically peculiar;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
We reconsidered the previous studies of properties of magnetic stars based on the latest data on average surface magnetic fields of 177 stars. New, corrected results have been obtained that allow a better understanding of the phenomenon of magnetic chemically peculiar stars.
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页码：66 / 79
页数：13
相关论文
共 81 条
[1]  
Hartoog M. R.(1977)undefined Astrophys. J. 212 723-undefined
[2]  
North P.(1984)undefined Astron. and Astrophys. 141 328-undefined
[3]  
Glagolevsky J. V.(2005)undefined Astrophysics 48 194-undefined
[4]  
Wolff S. C.(1981)undefined Astrophys. J. 244 221-undefined
[5]  
North P.(1984)undefined Astron. and Astrophys. Suppl. 58 387-undefined
[6]  
Cramer N.(1981)undefined Liege Intern. Astrophys. Colloquia 23 195-undefined
[7]  
Brown D. N.(1984)undefined Pis’ma Astron. Zh. 10 443-undefined
[8]  
Landstreet J. D.(1969)undefined Astrophys. J. Suppl. 18 347-undefined
[9]  
Thompson I.(1986)undefined Astrophys. Space Sci. Library 125 29-undefined
[10]  
Romanyuk I. I.(1987)undefined Astron. Zh. 64 360-undefined
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