Multiplicity of Chemically Peculiar Stars

被引：0
|
作者：
Hubrig, S. [1 ]
Gonzalez, J. F. [2 ]
Schoeller, M. [3 ]
机构：
[1] Astrophys Inst Potsdam, Sternwarte 16, D-14482 Potsdam, Germany
[2] Complejo Astron El Leoncito, RA-5400 San Juan, Argentina
[3] European So Observ, D-85748 Garching, Germany
来源：
BINARIES - KEY TO COMPREHENSION OF THE UNIVERSE | 2010年 / 435卷
关键词：
HGMN STARS; AP STARS; SPECTROSCOPIC BINARIES; MAGNETIC-FIELDS; AR-AUR; CATALOG; ELEMENTS; SYSTEM;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present the results of recent studies of binarity and multiplicity of chemically peculiar stars. The rate of binarity is strongly varying among different subclasses, which encompass magnetic Ap and Bp stars, HgMn stars, and metallic-line Am stars. The obtained observational results are discussed in the context of understanding the mechanisms generating chemical peculiarities and of A and B star formation in general.
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收藏
页码：257 / +
页数：3
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