Tidal Dwarf Galaxies: Their Present State and Future Evolution

Details Tidal Dwarf Galaxies: Their Present State and Future Evolution Tidal Dwarf Galaxies: Their Present State and Future Evolution

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998mcdg.proc..141f&link_type=abstract

The Magellanic Clouds and Other Dwarf Galaxies, Proceedings of the Bonn/Bochum-Graduiertenkolleg Workshop, held at the Physikzen

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Dynamics Of Dwarf Galaxies, Tidal Dwarf Galaxies, Galaxy Interaction

Scientific paper

Evolutionary synthesis models for Tidal Dwarf Galaxies (TDGs) are presented that allow to have varying proportions of young stars formed in the merger-induced starburst and of stars from the merging spirals' disks. Comparing model grids with observational data (see e.g. P.-A. Duc this conference for a review) we try to identify the present evolutionary state of TDGs. The influence of their specific metallicities as well as of the gaseous emission of actively star forming TDGs on their luminosity and colour evolution are studied.

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