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OB-stars as extreme condition test beds
Published online by Cambridge University Press: 12 July 2011
Abstract
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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- Copyright © International Astronomical Union 2011
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