n=5 Nonviscous Simulation

University of Illinois at Urbana-Champaign


Unlike the previous runs, we now use a value of n=5 in the initial equation of state.  The value of the characteristic strength of the magnetic field is shown in the top right image.  There is no viscosity. 

Note that the density of the star has been logged and normalized to the log of the initial central density.

Density Plots of Collapse

Fluid Flow during Collapse: Lagrangian Particle Representation

Temperature Plot

Scientific visualization by

University of Illinois at Urbana-Champaign
last updated 24 april 04 by kkc
Center for Theoretical Astrophysics---University of Illinois at Urbana-Champaign

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