Radiation from accretion discs

Statistics – Computation

Scientific paper

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Accretion Disks, Spectral Emission, Computation, Atmospheric Models, Hydrostatics, Radiation Distribution, Line Spectra

Scientific paper

The construction of self consistent model atmospheres for stationary accretion discs is reviewed and a method to calculate the corresponding hydrostatic structure and the radiation field is described. The importance of such models for the understanding of the continuum and the line emission as well as the necessity to construct the model in a self consistent way are discussed and demonstrated.

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