Synthetic spectra of dwarf nova disks

Details Synthetic spectra of dwarf nova disks Synthetic spectra of dwarf nova disks

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.236..217l&link_type=abstract

In ESA Recent Results on Cataclysmic Variables p 217-220 (SEE N86-20287 10-93)

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Accretion Disks, Cataclysmic Variables, Stellar Atmospheres, Stellar Models, Stellar Spectra, Atmospheric Models, Parameterization, Stellar Mass, Stellar Radiation

Scientific paper

Applying codes for stellar atmosphere computation, the ultraviolet and optical spectra of accretion disks in cataclysmic variables are investigated with assumed parameter sets characteristic of dwarf novae. As few and as simple assumptions as possible are made. The influence of the input parameters (mass, angle of inclination, assumed size, geometrical height) on the wavelength dependence of the radiation in optical and ultraviolet wavelengths is discussed.

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