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Based on the earlier work of Gunn and McCrea we model the formation ofglobular clusters in merging galaxies. Neutral hydrogen observations of dwarfirregular galaxies as well as more luminous systems are used to provide the keyparameters of the model. The observations indicate that clusters with the massof globular clusters should still be forming today. The model is incorporatedinto a phenomenological picture of galaxy evolution making use of a simplechemical evolution model. These results are compared to recent observations ofthe metallicity distributions of F and G stars from a recent large SDSS survey.The comparisons are consistent with an anisotropic collapse and merging of alarge number of dwarf irregular galaxies for the formation of the Galaxy.

Merger Induced Globular Cluster Formation and Galaxy Evolution