Ionization structure and mass loss for rapidly-rotating near main-sequence B stars

被引：0

作者：

Bjorkman, JE ^{[1
]}

Abbott, BP ^{[1
]}

机构：

[1] Univ Toledo, Dept Phys & Astron, Ritter Observ, Toledo, OH 43606 USA

来源：

BE PHENOMENON IN EARLY-TYPE STARS, PROCEEDINGS | 2000年 / 175卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using the wind-compressed disk model to determine the density and velocity of a rapidly rotating wind, we calculate the 2-D ionization structure and corresponding line profiles. We find that previous estimates of the mass-loss rate based on spherically symmetric models may be a factor of 5-10 too small.

引用

页码：632 / 635

页数：2

共 6 条

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