Proceedings of the Workshop
"The Magellanic Clouds and Other Dwarf Galaxies"
of the Bonn/Bochum-Graduiertenkolleg

dSph Satellite Galaxies without Dark Matter:

a Study of Parameter Space

Pavel Kroupa

 [Fig. 1]
Fig. 1. The time t=τ50, when (M/L)obs(t)≥50, is plotted against orbital eccentricity for a number of simulations with Msat=107 Msun and RPl=300 pc, as defined in the key
[Fig. 2]
Fig. 2. Initial satellite mass as a function of initial characteristic satellite radius
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First version: 14thJuly,1998
Last update: 28thSeptember,1998
Jochen M. Braun   &   Tom Richtler
 (E-Mail: jbraun|richtler@astro.uni-bonn.de)