Viscous evolution of accretion discs in the quiescence of dwarf novae

Details Viscous evolution of accretion discs in the quiescence of dwarf novae Viscous evolution of accretion discs in the quiescence of dwarf novae

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.241..259m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 241, Nov. 15, 1989, p. 259-280.

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Accretion Disks, Computational Astrophysics, Dwarf Novae, Stellar Evolution, Viscosity, Brightness Temperature, Emission Spectra, Mass Transfer, Stellar Mass, Temperature Gradients, X Ray Sources

Scientific paper

Viscous evolution of accretion disks in the quiescence of dwarf novae is investigated semi-analytically. There are two key factors: the inward flow of the initial mass in the disk and the diffusion of the material added into the disk. The results are compared with the brightness temperature distributions obtained by the eclipse mapping of Z Cha and OY Car. The functional form of the viscosity parameter a, its values, the types of outbursts, and the application to soft X-ray transients are discussed.

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