VARIABILITY AND THEORETICAL UPPER LIMIT OF THE MASS-LOSS RATE IN OB-STARS

被引：0
|
作者：
VILKOVISKIJ, EY
TAMBOVTSEVA, LV
机构：
来源：
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1992年 / 94卷 / 01期
关键词：
EARLY-TYPE STARS; MASS LOSS; STELLAR WINDS;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Solutions of the stellar wind equations for 70 0-type and 19 B-type individual stars are presented. The calculated mass loss rates M, terminal velocities v(infinity) and line profiles are compared with the observed ones. It is shown that a theoretical upper limit of the mass loss rate M(crit) exists. Wind variability in connection with M(crit) is discussed.
引用
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页码：109 / 120
页数：12
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