Radiative Transfer in Axial Symmetry

Details Radiative Transfer in Axial Symmetry Radiative Transfer in Axial Symmetry

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1171..359k&link_type=abstract

RECENT DIRECTIONS IN ASTROPHYSICAL QUANTITATIVE SPECTROSCOPY AND RADIATION HYDRODYNAMICS: Proceedings of the International Confe

Computer Science

Numerical Analysis

Radiative Transfer, Stellar Winds, Numerical Analysis, Radiative Transfer, Scattering, Mass Loss And Stellar Winds, Numerical Approximation And Analysis

Scientific paper

We present a numerical code for the solution of the radiative transfer problem in moving media. The used method is based on the axial symmetry approximation. The output from the code is the overall spectrum of the object and the intensity map. The code is appropriate for the description of the radiation field in extended stellar atmospheres, rapidly rotating stars, stellar winds and disks around stars. It is also applicable for the disks of cataclysmic variables.

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