Abstract
In a 1st step I present results from our new set of evolutionary synthesis models for Simple (= single burst) Stellar Populations (SSPs) of various metallicities, and in a 2nd step I combine these results with the information we have about the redshift evolution of spiral galaxies’ ISM abundances. The aim is to provide a grid of color and luminosity distibutions of any secondary GC population formed at some time in the past in those mergers for comparison with observations.
Original language | English |
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Title of host publication | In: Procs of Extragalactic Star Clusters - IAU Symposium 207 |
Publisher | Astronomical Society of the Pacific |
Pages | 642-8 |
Publication status | Published - 2002 |