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

Starbursts in dwarf galaxies:

Blown out or blown away?

Mordecai-Mark Mac Low and Andrea Ferrara


[Fig. 1]
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: 09thAugust,1998
Last update: 28thSeptember,1998

Jochen M. Braun   &   Tom Richtler
 (E-Mail: jbraun|richtler@astro.uni-bonn.de)