The young star cluster system of the Antennae galaxies

Peter Anders*, Uta Fritze, Richard de Grijs

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

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Abstract

The study of young star cluster (YSC) systems, preferentially in starburst and merging galaxies, has seen great interest in the recent past, as it provides important input to models of star formation. However, even some basic properties (such as the luminosity function; LF) of YSC systems are still being debated. Here, we study the photometric properties of the YSC system in the nearest major merger system, the Antennae galaxies. We find evidence for the existence of a statistically significant turnover in the LF.

Original languageEnglish
Pages (from-to)305-308
Number of pages4
JournalAstrophysics and Space Science
Volume324
Issue number2-4
DOIs
Publication statusPublished - Nov 2009
Externally publishedYes

Bibliographical note

Copyright the Author(s) 2009. Version archived for private and non-commercial use with the permission of the author/s and according to publisher conditions. For further rights please contact the publisher.

Keywords

  • galaxies: NGC 4038/39
  • methods: data analysis
  • star clusters: general

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