On the wind momentum problem of O-type stars in the galaxy

被引：0
|
作者：
G. Israelian
K. Vyverman
机构：
[1] Insituto de Astrofisica de Canarias,Astronomy Group
[2] Vrije Universiteit Brussel,undefined
来源：
Astrophysics and Space Science | 1997年 / 254卷
关键词：
Mass Loss Rate; Radiative Force; Stellar Wind; Terminal Velocity; Atomic Data;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
We have examined the wind momentum problem of O-type stars in the Galaxy. It is shown that the discrepancy between theoretical and empirical mass loss rates and terminal velocities can be reversed by using recently updated values of force multiplier parameters. With these new values, the momentum problem found by former investigators is reversed so that there now appears to be more than enough radiation force in order to accelerate the stellar winds of a sample of Galactic O-type stars.
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页码：51 / 60
页数：9
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