On Properties of Main Sequence Magnetic Stars

被引：28
作者：
Glagolevskij, Yu. V. [1 ]
机构：
[1] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Russia
来源：
ASTROPHYSICAL BULLETIN | 2019年 / 74卷 / 01期
基金：
英国科研创新办公室;
关键词：
stars: magnetic fields; stars: chemically peculiar; CHEMICALLY PECULIAR STARS; AP STARS; EFFECTIVE TEMPERATURE; OPEN CLUSTERS; FIELDS; EVOLUTION; ROTATION; PARAMETERS; PHOTOMETRY; BEHAVIOR;
D O I：
10.1134/S1990341319010073
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
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.
引用
收藏
页码：66 / 79
页数：14
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