Maximum mass-loss rates of line-driven winds of massive stars: The effect of rotation and an application to ηCarinae
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20040090/pdf
Reference25 articles.
1. Maximum mass-loss rates of line-driven winds of massive stars
2. Equatorial disk formation around rotating stars due to Ram pressure confinement by the stellar wind
3. Radiation-driven winds in Of stars
4. Radiatively Driven Winds and the Shaping of Bipolar Luminous Blue Variable Nebulae
5. Abbott Wave–triggered Runaway in Line‐driven Winds from Stars and Accretion Disks
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