Numerical Simulation of Accretion Discs in Close Binary Systems andDiscovery of Spiral Shocks |
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| Authors: | Takuya Matsuda Makoto Makita Hidekazu Fujiwara Takizo Nagae Kei Haraguchi Eiji Hayashi HMJ Boffin |
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| Institution: | (1) Department of Earth and Planetary Sciences, KobeUniversity, Kobe, Japan;(2) Department of Earth and Planetary Sciences, KobeUniversity, Kobe, Japan;(3) Royal Observatory, Brussel, Belgium |
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| Abstract: | The history of hydrodynamic numerical simulations for accretion disks in close binary systems is reviewed, in which emphasis
is placed, in particular, on the facts that spiral shock waves were numerically found in 1986 by researchers including one
of the present authors and that spiral structure was discovered in IP Pegasi in 1997 by Steeghs et al. The results of our two and three-dimensional numerical simulations in recent years are then summarized, with comparison being
made with observations.
This revised version was published online in July 2006 with corrections to the Cover Date. |
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