Predicting Metallicities and Color Distributions for Secondary GCs Forming in Spiral Galaxy Mergers at Various Redshifts

Details Predicting Metallicities and Color Distributions for Secondary GCs Forming in Spiral Galaxy Mergers at Various Redshifts Predicting Metallicities and Color Distributions for Secondary GCs Forming in Spiral Galaxy Mergers at Various Redshifts

2001-06-07

arxiv.org/abs/astro-ph/0106129v1

Astronomy and Astrophysics

Astrophysics

6 pages, 1 Fig. To appear in IAU Symp. 207 {\sl Extragalactic Star Clusters}, eds. E. K. Grebel, D. Geisler, D. Minniti

Scientific paper

In a 1$^{\rm st}$ step I present results from our new set of evolutionary synthesis models for Simple (= single burst) Stellar Populations ({\bf SSP}s) of various metallicities, and in a 2$^{\rm nd}$ 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.

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