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Radiative transfer in axial symmetry
Published online by Cambridge University Press: 08 March 2006
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.
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- Research Article
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- © EAS, EDP Sciences, 2006