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.