Title of article
Line profiles of OB star winds using a Monte Carlo method
Author/Authors
Brankica Surlan، نويسنده , , Jiri Kubat، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2010
Pages
2
From page
214
To page
215
Abstract
The solution of the radiative transfer in an expanding atmospheres using the Monte Carlo method is presented. We applied our method to winds of several OB stars. In our calculation, the velocity and density structure is assumed to be given. Selected line profiles are shown.
Keywords
line: formation , outflows , radiative transfer , stars: winds
Journal title
Proceedings of the International Astronomical Union
Serial Year
2010
Journal title
Proceedings of the International Astronomical Union
Record number
667845
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