On the computation of accretion disk spectra

Details On the computation of accretion disk spectra On the computation of accretion disk spectra

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.130..337l&link_type=abstract

(IAU, DFG, and Bayerisches Staatsministerium für Unterricht und Kultus, Colloquium on Cataclysmic Variables, Recent Multi-Freque

Astronomy and Astrophysics

Astrophysics

3

Accretion Disks, Dwarf Novae, Stellar Mass Accretion, Stellar Spectra, Stellar Atmospheres, Stellar Temperature

Scientific paper

Spectra of accretion disks in dwarf novae and some nova-like stars have been computed. Many simplifications to the general model of the nature of a cataclysmic variable are needed to make the system numerically tractable. The necessity, justification, and implications of such simplifications are discussed together with the influences of some system parameters on the disk radiation.

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