Accretion Disk Dynamics in the Interacting Binary White Dwarfs

Details Accretion Disk Dynamics in the Interacting Binary White Dwarfs Accretion Disk Dynamics in the Interacting Binary White Dwarfs

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...183.5209s&link_type=abstract

American Astronomical Society, 183rd AAS Meeting, #52.09; Bulletin of the American Astronomical Society, Vol. 25, p.1373

Astronomy and Astrophysics

Astronomy

Scientific paper

We present preliminary results of a 2 dimensional simulation of an interacting binary white dwarf (IBWD) system. The IBWDs are characterized by extreme mass ratios q~0.02 and nearly pure helium accretion disks. The viscous fliud flow is modelled using the numerical method of smoothed particle hydrodynamics (SPH), and the equations of motion are solved in the inertial reference frame centered at the system center of mass.

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