OB-stars as extreme condition test beds
Solar and Stellar Astrophysics
2015-05-19 v1
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.
Cite
@article{arxiv.1009.0364,
title = {OB-stars as extreme condition test beds},
author = {Joachim Puls and Jon O. Sundqvist and Jorge G. Rivero González},
journal= {arXiv preprint arXiv:1009.0364},
year = {2015}
}
Comments
To be published in the proceedings book of the IAUS 272, Cambridge University Press. Editors C. Neiner, G. Wade, G. Meynet and G. Peters