Fig. 1.
Density distributions for models with the given initial visible masses
Mg and mechanical luminosities Lm at
a time of 100 Myr, with the values of density given at the top of
the figure.
Note that energy input ended at 50 Myr.
Lengths are given in terms of the exponential scale height for each model,
with values quoted in the Figure
Links (back/forward) to:
First version: | 09th | August, | 1998
|
Last update: | 28th | September, | 1998
|
Jochen M. Braun &
Tom Richtler
(E-Mail: jbraun|richtler@astro.uni-bonn.de)