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

Tidal Dwarf Galaxies:

Their Present State and Future Evolution

Uta Fritze - v. Alvensleben and Pierre-Alain Duc


[Fig. 1a] [Fig. 1b]
Fig. 1. a) Relative contribution of gaseous emission to broad band colours UBVRIJHK 1 Myr after the onset of bursts of various strengths.
b) Decomposition of the total gaseous emission contribution for a strong burst (Fig. 1a) into contributions from lines and continuum

[Fig. 2a] [Fig. 2b]
Fig. 2. Two colour diagrams for a) (B-V) vs. (V-R) (left or above panel) and
b) (B-V) vs. (V-K) (right or below panel), respectively

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First version: 14thAugust,1998
Last update: 27thSeptember,1998

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