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Connections between MWG Star Clusters and Dwarf Galaxies

Published online by Cambridge University Press:  05 March 2015

Kim A. Venn
Kim A. Venn*
Affiliation:
University of Victoria, PO Box 3055 STN CSC, Victoria, BC, CanadaV8W 3P6 email: kvenn@uvic.ca
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It seems that in the past decade, there have been two paradigm shifts regarding star clusters. Firstly, the observational evidence for multiple stellar populations requires more extended and often complex star formation histories in star clusters. Secondly, theoretical models that form globular clusters in dwarf galaxies that are accreted at very early epochs (z > 5) are able to reproduce the age-metallicity relations observed. For the accretion scenario to be viable, globular clusters should also resemble the chemistry of at least some dwarf galaxies.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 275 - 277
Copyright
Copyright © International Astronomical Union 2015 

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