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The properties of nuclear star clusters and their host galaxies

Published online by Cambridge University Press:  11 March 2020

Anil C. Seth Open the ORCID record for Anil C. Seth [Opens in a new window] ,
Nadine Neumayer  and
Torsten Böker
Anil C. Seth
Affiliation:
University of Utah, Salt Lake City email: aseth@astro.utah.edu
Nadine Neumayer
Affiliation:
Max Planck Institute for Astronomy, Heidelberg
Torsten Böker
Affiliation:
European Space Agency, Space Telescope Science Center, Baltimore
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Abstract

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Nuclear star clusters are found at the centers of most galaxies. They are the densest stellar systems in the Universe, and thus have unique and interesting stellar dynamics. We review how common nuclear star clusters are in galaxies of different masses and types, and then discuss the typical properties of NSCs. We close by discussing the formation of NSCs, and how a picture is emerging of different formation mechanisms being dominant in lower and higher mass galaxies.

Keywords

galaxies: nucleusgalaxies: evolutiongalaxies: star clusters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S351: Star Clusters: From the Milky Way to the Early Universe , May 2019 , pp. 13 - 18
Copyright
© International Astronomical Union 2020

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