Maximum mass-loss rates of line-driven winds of massive stars
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20030349/pdf
Reference33 articles.
1. The theory of radiatively driven stellar winds. II - The line acceleration
2. Equatorial disk formation around rotating stars due to Ram pressure confinement by the stellar wind
3. Radiation-driven winds in Of stars
4. Runaway of Line-driven Winds toward Critical and Overloaded Solutions
Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Exploration of spin-down rate of neutron stars in high-mass X-ray binaries;Monthly Notices of the Royal Astronomical Society;2016-02-26
2. Upper limit for the mass loss rate of rapidly rotating single main-sequence O9-B4 stars;Astronomy Letters;2010-10-19
3. Maximum mass-loss rates of line-driven winds of massive stars: The effect of rotation and an application to ηCarinae;Astronomy & Astrophysics;2004-04-09
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