Searching for flickering statistics in T CrB
arXiv:0911.3804 · doi:10.1111/j.1365-2966.2009.16068.x
Abstract
We analyze -band photometry of the aperiodic variability in T CrB. By applying a simple idea of angular momentum transport in the accretion disc, we have developed a method to simulate the statistical distribution of flare durations with the assumption that the aperiodic variability is produced by turbulent elements in the disc. Both cumulative histograms with Kolmogorov-Smirnov tests, and power density spectra are used to compare the observed data and simulations. The input parameters of the model and are correlated on a certain interval and the most probable values are an inner disc radius of cm and a viscosity of . The disc is then weakly truncated. We find that the majority of turbulent events producing flickering activity are concentrated in the inner parts of the accretion disc.
9 pages, 10 figures, accepted for publication in MNRAS
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Cited by in corpus (16)
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