Young Star Clusters: Clues to Galaxy Formation and Evolution

Peter Anders, Uta Fritze-V. Alvensleben, Richard de Grijs
2004 Symposium - International astronomical union  
Young clusters are observed to form in a variety of interacting galaxies and violent starbursts, a substantial number resembling the progenitors of the well-studied globular clusters in mass and size. By studying young clusters in merger remnants and peculiar galaxies, we can therefore learn about the violent star formation history of these galaxies. We present a new set of evolutionary synthesis models of our GALEV code specifically developed to include the gaseous emission of presently
more » ... star clusters, and a new tool that allows to determine individual cluster metallicities, ages, extinction values and masses from a comparison of a large grid of modelSpectralEnergyDistributions (SEDs) with multi-color observations. First results for the newly-born clusters in NGC 1569 are presented.
doi:10.1017/s0074180900197529 fatcat:wbccttr2bbarnocycivirio23m