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19952006
most citedNGC 3310 and Its Tidal Debris: Remnants of Galaxy Evolution

18 citations · 32 across the 13 of their papers we have counts for

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Showing 2003Show all

9 papers · 1 filter

astro-ph2003

Secondary Globular Cluster Populations

Uta Fritze -- v. Alvensleben

Globular Cluster (GC) systems of most early-type galaxies show bimodal optical color distributions, yet their Luminosity Functions (LFs) look like simple Gaussians with turn-over m…

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-ph2003

Chemically consistent evolution of galaxies: II. Spectrophotometric evolution from zero to high redshift

Jens Bicker, Uta Fritze - v. Alvensleben, Claudia S. Moeller +1

We present a new generation of chemically consistent evolutionary synthesis models for galaxies of various spectral types from E through Sd. The models follow the chemical enrichme…

astro-ph2003★ 1 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-ph2003★ 1 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…