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Radiative transfer in axial symmetry

Published online by Cambridge University Press:  08 March 2006

Ph. Stee ,
D. Korčáková  and
J. Kubát
D. Korčáková
Affiliation:
Astronomický Ústav, Akademie věd České Republiky, 251 65 Ondřejov, Czech Republic
J. Kubát
Affiliation:
Astronomický Ústav, Akademie věd České Republiky, 251 65 Ondřejov, Czech Republic
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Abstract

We present a method for solving the radiative transfer equation in axial symmetry both in static case and in moving media. A usage of this method is shown here for stellar atmospheres, stellar winds, and accretion discs. The effects of limb darkening and stellar rotation are discussed, too.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 18: Radiative Transfer and Applications to Very Large Telescopes , 2006 , pp. 67 - 75
Copyright
© EAS, EDP Sciences, 2006

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