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Physics of mass loss in massive stars

We review potential mass-loss mechanisms in the various evolutionary stages of massive stars, from the well-known line-driven winds of O-stars and BA-supergiants to the less-understood winds from Red Supergiants. We discuss optically thick winds from Wolf-Rayet stars and Very Massive Stars, and the hypothesis of porosity-moderated, continuum-driven mass loss from stars formally exceeding the Eddington limit, which might explain the giant outbursts from Luminous Blue Variables. We finish this review with a glance on the impact of rapid rotation, magnetic fields and small-scale inhomogeneities in line-driven winds.

preprint2014arXivOpen access
J. PulsJ. O. SundqvistN. Markova
astro-ph.SR
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Open access3 authors1 topic
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J. PulsJ. O. SundqvistN. Markova

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