Outflowing disk formation in B[e] supergiants due to rotation and bi-stability in radiation driven winds
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20052686/pdf
Reference23 articles.
1. The theory of radiatively driven stellar winds. II - The line acceleration
2. Bjorkman, J. E. 1998, in B[e]stars, ed. A. M. Hubert, & C. Jascheck, ASSl 233 (Dordrecht: Kluwer), 189
3. Radiation-driven winds in Of stars
4. The effect of oblateness and gravity darkening on the radiation driving in winds from rapidly rotating B stars
5. The Influence of Rotation in Radiation‐driven Wind from Hot Stars: New Solutions and Disk Formation in Be Stars
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