The UV-delay in dwarf nova outbursts as a consequence of details of the accretion disks' vertical stratification

Details The UV-delay in dwarf nova outbursts as a consequence of details of the accretion disks' vertical stratification The UV-delay in dwarf nova outbursts as a consequence of details of the accretion disks' vertical stratification

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...247..393d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 247, no. 2, July 1991, p. 393-398.

Astronomy and Astrophysics

Astronomy

2

Accretion Disks, Dwarf Novae, Stellar Models, Ultraviolet Astronomy, Bolometers, Light Curve, Spectral Emission, Stellar Luminosity

Scientific paper

Results of time dependent model calculations are presented for the evolution of dwarf nova accretion disks with self-consistent viscosity description. New features in the stationary vertical stratification, due to this modeling of viscosity, make it possible to explain quantitatively the halt in the visual wavelength band in the rise to maximum during a dwarf nova outburst. The same features are also responsible for the UV-delay during rise to maximum.

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