OB-stars as extreme condition test beds

Details OB-stars as extreme condition test beds OB-stars as extreme condition test beds

2010-09-02

arxiv.org/abs/1009.0364v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

To be published in the proceedings book of the IAUS 272, Cambridge University Press. Editors C. Neiner, G. Wade, G. Meynet and

Scientific paper

Massive stars are inherently extreme objects, in terms of radiation, mass loss, rotation, and sometimes also magnetic fields. Concentrating on a (personally biased) subset of processes related to pulsations, rapid rotation and its interplay with mass-loss, and the bi-stability mechanism, we will discuss how active (and normal) OB stars can serve as appropriate laboratories to provide further clues.

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