Continuous energy distributions of accretion discs

Details Continuous energy distributions of accretion discs Continuous energy distributions of accretion discs

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...251..117s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 251, no. 1, Nov. 1991, p. 117-132. Research supported by German-Israeli Founda

Astronomy and Astrophysics

Astrophysics

32

Accretion Disks, Cataclysmic Variables, Spectral Energy Distribution, White Dwarf Stars, Astronomical Models, Novae, Radiative Transfer, Stellar Atmospheres

Scientific paper

A model to calculate the continuum radiation emerging from accretion disks is presented. The method solves the disk equations in a self-consistent way after the basic assumptions are made. The comparison with observations shows good agreement over a wide range of wavelengths. The reasons for the success of the model are analyzed and it is shown that the basic reason for this achievement is the fact that the solution is selfconsistent.

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