Searching for Observed Distribution of Flickering Flare Duration in T CrB

Details Searching for Observed Distribution of Flickering Flare Duration in T CrB Searching for Observed Distribution of Flickering Flare Duration in T CrB

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..330..361d&link_type=abstract

The Astrophysics of Cataclysmic Variables and Related Objects, Proceedings of ASP Conference Vol. 330. Edited by J.-M. Hameury a

Astronomy and Astrophysics

Astrophysics

Scientific paper

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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