Stationary Solutions for the Supersonic Wind Accretion

Details Stationary Solutions for the Supersonic Wind Accretion Stationary Solutions for the Supersonic Wind Accretion

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999sf99.proc..407o&link_type=abstract

Star Formation 1999, Proceedings of Star Formation 1999, held in Nagoya, Japan, June 21 - 25, 1999, Editor: T. Nakamoto, Nobeyam

Physics

Scientific paper

We discuss the results of numerical simulation of the hydrodynamic Bondi-Hoyle accretion on the basis of the high-resolution numerical scheme. Both axisymmetric and plane cases are considered. Axisymmetric accretion problem turns out to have stationary solutions for all parameters. For plane accretion, stationary solutions are found in certain cases even for sinusoidally perturbed and strongly nonuniform winds. Nonstationary phenomena do exist but they are not very violent and may sometimes be attributed to numerical as well as physical reasons.

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