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Paper: Emission from a Flat Accretion Disk with a Finite Radius in a Black-Body Approximation
Volume: 362, The Seventh Pacific Rim Conference on Stellar Astrophysics
Page: 138
Authors: Baklanov, A.V.; Andronov, I.L.
Abstract: 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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