Emission from a Flat Accretion Disk with a Finite Radius in a Black-Body Approximation

Details Emission from a Flat Accretion Disk with a Finite Radius in a Black-Body Approximation Emission from a Flat Accretion Disk with a Finite Radius in a Black-Body Approximation

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..362..138b&link_type=abstract

The Seventh Pacific Rim Conference on Stellar Astrophysics, ASP Conference Series, Vol. 362, Proceedings of the conference held

Astronomy and Astrophysics

Astrophysics

Scientific paper

Results of numerical modeling of an accretion disk with a finite radius using a local black-body approximation are presented. The dependences of the luminosity, color indices of the system parameters and spectral energy distribution on the main system parameters have been determined. The contributions of the shell sources to the total disk luminosity and its spectral energy distribution have been computed. The algorithm and program "BBAD" are aimed for modeling of multi-color observations of cataclysmic variables.

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