Late density structure on larger scale
A larger view of the density structure in
Model 14A at a later time (in a calculation where no jet was
initiated), 15.63 s. The inner disk with its higher density
is unresolved here. The density along the
polar axis has declined to 10**4 g/cm**3, approximately the mean
density of the star.
Above picture: Gzipped Postscript
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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.