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
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
Journal title :
Proceedings of the International Astronomical Union