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From Young to Old: Spectral Models for Star Cluster Systems
Uta Fritze -- v. Alvensleben, Peter Anders, Richard de Grijs
Evolutionary synthesis models for star clusters of various metallicities including gaseous emission during the lifetime of the ionising stars are used to model star cluster systems…
Young star clusters: Clues to galaxy formation and evolution
P. Anders, U. Fritze--v. Alvensleben, R. de Grijs
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 cluste…
Young star clusters: Metallicity tracers in external galaxies
P. Anders, U. Fritze--v. Alvensleben, R. de Grijs
Star cluster formation is a major mode of star formation in the extreme conditions of interacting galaxies and violent starbursts. These newly-formed clusters are built from recycl…
Young star clusters: Progenitors of globular clusters!?
P. Anders, U. Fritze--v. Alvensleben, R. de Grijs
Star cluster formation is a major mode of star formation in the extreme conditions of interacting galaxies and violent starbursts. Young clusters are observed to form in a variety…
Multi-color observations of Young Star Clusters
P. Anders, U. Fritze--v. Alvensleben, R. de Grijs
We present a new set of evolutionary synthesis models of our GALEV code, specifically developed to include the gaseous emission of presently forming star clusters, in combination w…