Title of article
OB-stars as extreme condition test beds
Author/Authors
Joachim Puls، نويسنده , , Jon O. Sundqvist، نويسنده , , Jorge G. Rivero Gonzalez، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2010
Pages
12
From page
554
To page
565
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 bistability mechanism, we will discuss how active (and normal) OB stars can serve as appropriate laboratories to provide further clues.
Keywords
stars: rotation , stars: winds , outflows , Hydrodynamics , instabilities , line: formation , stars: abundances , stars: early-type , stars: evolution , stars: oscillations , stars: mass loss
Journal title
Proceedings of the International Astronomical Union
Serial Year
2010
Journal title
Proceedings of the International Astronomical Union
Record number
667948
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