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Paper: Searching for Observed Distribution of Flickering Flare Duration in T CrB
Volume: 330, The Astrophysics of Cataclysmic Variables and Related Objects
Page: 361
Authors: Dobrotka, A.; Hric, L.; Mikus, M.
Abstract: On the basis of the assumption that the manifestations of turbulence in the accretion disc of CVs are the observed flickering flares, we assumed the relative frequency of events as a function of their duration and of system parameters. The best approach of our simulation to observation for T CrB is obtained for parameters α = 0.1 and Macc = 1020 g s−1.
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