Ph. Stee (ed)
EAS Publications Series, 18 (2006) 67-75
Radiative transfer in axial symmetry
Astronomický Ústav, Akademie věd České
Republiky, 251 65 Ondřejov, Czech Republic
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.
© EAS, EDP Sciences, 2006