Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...211..131l&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 211, no. 1, Feb. 1989, p. 131-155.
Astronomy and Astrophysics
Astrophysics
45
Absorption Spectra, Accretion Disks, Cataclysmic Variables, Ultraviolet Spectra, Visible Spectrum, Dwarf Novae, Line Spectra, Optical Thickness, Stellar Atmospheres, Stellar Spectrophotometry, White Dwarf Stars
Scientific paper
Continuous spectra and absorption line spectra of accretion disks in cataclysmic variables in the range between 100 and 100,000 A were computed, with the computations restricted to stationary optically thick, but geometrically thin, accretion disks with simplified atmospheres. A much larger parameter range was covered than those covered by previous investigators, with respect to the influence of the mass of the white dwarf, the inner and the outer disk radii, the mass transfer rate, and the angle of inclination. The comparison of these computations with the results of similar computations by other groups revealed discrepancies in the results, which are larger than should be expected from merely making somewhat different assumptions underlying the computations.
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