Chemical composition of the He-w stars HD 37058, 212454, and 224926

被引：0
|
作者：
Yu. V. Glagolevskij
V. V. Leushin
G. A. Chountonov
机构：
[1] Russian Academy of Sciences,Special Astrophysical Observatory
来源：
Astrophysical Bulletin | 2007年 / 62卷
关键词：
97.30.Fi; 97.10.Ld;
D O I：
暂无
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摘要：
Our spectrophotometric analysis of the atmospheres of HD 37058, HD 212454, and HD 224926 shows these objects to be typical He-w stars with close-to-zero microturbulence velocities, very different magnetic fields, and wide scatter of chemical anomalies. However, one of the main manifestations of separation is that helium moves from the outer layers of the atmosphere into the star’s interior.
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页码：319 / 330
页数：11
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