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2000MNRAS.316..906M - Mon. Not. R. Astron. Soc., 316, 906-916 (2000/August-3)
Two- and three-dimensional numerical simulations of accretion discs in a close binary system.
MAKITA M., MIYAWAKI K. and MATSUDA T.
Abstract (from CDS):
Recently, Steeghs, Harlaftis & Horne found the first convincing evidence for spiral structure in the accretion disc of the eclipsing dwarf nova binary IP Pegasi, using the technique known as Doppler tomography. Although the Mach numbers in present calculations are rather low, we may claim that the spiral structure that we discovered in earlier numerical simulations is now found observationally.
Abstract Copyright: 2000, Royal Astronomical Society
Journal keyword(s): accretion, accretion discs - hydrodynamics - shock waves - methods: numerical - binaries: close
Simbad objects: 3
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