Line profiles of OB star winds using a Monte Carlo method

Details Line profiles of OB star winds using a Monte Carlo method Line profiles of OB star winds using a Monte Carlo method

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..272..214s&link_type=abstract

Active OB stars: structure, evolution, mass loss, and critical limits, Proceedings of the International Astronomical Union, IAU

Astronomy and Astrophysics

Astronomy

Radiative Transfer, Line: Formation, Stars: Winds, Outflows

Scientific paper

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.

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