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Abstract: Massive stars are inherently extreme objects, in terms of radiation, massloss, rotation, and sometimes also magnetic fields. Concentrating on apersonally biased subset of processes related to pulsations, rapid rotationand its interplay with mass-loss, and the bi-stability mechanism, we willdiscuss how active and normal OB stars can serve as appropriate laboratoriesto provide further clues.



Autor: Joachim Puls, Jon O. Sundqvist, Jorge G. Rivero González

Fuente: https://arxiv.org/







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