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20022005
most citedYoung star clusters: Metallicity tracers in external galaxies

1 citations · 4 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph20051 cited

Nearby star cluster formation: Probes of cosmological galaxy evolution

P. Anders, R. de Grijs, U. Fritze-v. Alvensleben

(abridged) The old Star Cluster (SC) systems surrounding any sofar investigated galaxy represent a powerful tool for the understanding of the cosmological evolution of their host g…

astro-ph2003

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…

astro-ph20031 cited

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…

astro-ph20031 cited

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…

astro-ph2003

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…

astro-ph20021 cited

Analysing Multi-Color Observations of Young Star Clusters in Mergers

Peter Anders, Uta Fritze--v. Alvensleben, Richard de Grijs

We present a new evolutionary synthesis (ES) tool specifically developed for the analysis of multi-color data of young star clusters (YSCs) in interacting galaxies. Our ESO/ST-ECF…