Physics
Scientific paper
Mar 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..361..337g&link_type=abstract
Active OB-Stars: Laboratories for Stellar and Circumstellar Physics, ASP Conference Series, Vol. 361, Proceedings of the confere
Physics
Scientific paper
From a theoretical point of view models for OB stars suffer from a variety of instabilities operating at subphotospheric levels. Their occurrence as a function of and dependence on stellar parameters and evolutionary state will be reviewed. We shall report on theoretical results concerning the final fate of violently unstable objects. The physics of the instability mechanisms will be commented on.
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