Shock waves in accretion disks in close binary stars.

Details Shock waves in accretion disks in close binary stars. Shock waves in accretion disks in close binary stars.

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008uvun.conf..118b&link_type=abstract

"Ultraviolet Universe II, Proceedings of the All-Russian Conference "UV Universe-2008" May 19-20, 2008, Moscow, Russia, Shustov,

Physics

Scientific paper

Three-dimensional numerical simulations of the gas dynamics are used to study the flow pattern in a close binary system after it has reached the steady-state accretion regime. The special attention is paid at physics of accretion disks in binary systems and particularly at waves in disks. It is shown that in systems with stationary accretion disks there are shock waves: the "hot line" formed due to interaction between the circumdisk halo and the stream from the inner Lagrange point L1, and two arms of the tidal shock. Possible observational manifestations of these shocks are discussed.

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