Accretion Disk Models for Symbiotic Stars - Part Two - Time-Dependent Accretion Disks

Details Accretion Disk Models for Symbiotic Stars - Part Two - Time-Dependent Accretion Disks Accretion Disk Models for Symbiotic Stars - Part Two - Time-Dependent Accretion Disks

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...163...61d&link_type=abstract

Astronomy and Astrophysics, Vol.163, NO.1&2/JULII, P. 61, 1986

Astronomy and Astrophysics

Astrophysics

30

Scientific paper

It is shown that the lightcurves of symbiotic stars can be understood as
being due to the time dependent evolution of accretion disks around main
sequence stars, governed by the same accretion disk instability as may
be responsible for dwarf novae outbursts.

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