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Influence of X-ray radiation on the non-LTE wind models of O-type stars

Published online by Cambridge University Press:  01 August 2006

Jiří Krtička
Jiří Krtička*
Affiliation:
Institute for Theoretical Physics and Astrophysics, Faculty of Sciences, Masaryk University, Kotlarska 2, CZ – 611 37 Brno, Czech Republic email: krticka@physics.muni.cz
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Abstract

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We study the influence of shock X-ray emission on the structure of non-LTE wind models of O-type stars.

Keywords

stars: early-typestars: atmospheresstars: windsoutflows
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 212
Copyright
Copyright © International Astronomical Union 2007