Density structure for low viscosity run
Density structure at 7.52 s in the low viscosity run, Model 14B. Note
the higher density contrast and more massive disk than in the
calculation with high viscosity (Fig. 8). The
opening angle of the accretion column is also larger and viscosity
induced outflows are absent.
Above picture: Gzipped Postscript | PDF | GIF
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Andrew MacFadyen-
andrew@ucolick.org - October 20, 1998
Kerr Hall 237B - (831)459-2774
Lick Observatory and Department of Astronomy and Astrophysics
UC Santa Cruz, CA 95064, U.S.A.