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arXiv · 1408.1924

Estimation of alpha-viscosity coefficient from observations of nonstationary disk accretion

G. S. Bisnovatyi-Kogan·A. S. Klepnef·F. Giovannelli
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Abstract

The optical behaviour of the Be star in the high mass X-ray transient A0535+26/HDE245770 shows that at the periastron typically there is an enhancement in the luminosity of order 0.05 to few tenths mag, and the X- ray outburst happens about 8 days after the periastron. We construct a quantitative model of this event, basing on a nonstationary accretion disk behavior, connected with a high ellipticity of the orbital motion. We explain the observed time delay between the peaks of the optical and X-ray outbursts in this system by the time of radial motion of a matter in the accretion disk, after increase of the mass flux in the vicinity of a periastral point in the binary. This time is determined by the turbulent viscosity, with the parameter $ \alpha=0.1-0.3$, estimated from the comparison of the model with observational data

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G. S. Bisnovatyi-Kogan, A. S. Klepnef, F. Giovannelli. 2014-08-08. Estimation of alpha-viscosity coefficient from observations of nonstationary disk accretion. https://arxiv.org/abs/1408.1924

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