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Integrated spectroscopy of extragalactic Globular Clusters

Published online by Cambridge University Press:  11 March 2020

Charli M. Sakari Open the ORCID record for Charli M. Sakari [Opens in a new window]
Charli M. Sakari*
Affiliation:
Department of Astronomy, University of Washington, SeattleWA98195-1580, USA email: sakaricm@uw.edu
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Abstract

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Integrated light (IL) spectroscopy enables studies of stellar populations beyond the Milky Way and its nearest satellites. In this paper, I will review how IL spectroscopy reveals essential information about globular clusters and the assembly histories of their host galaxies, concentrating particularly on the metallicities and detailed chemical abundances of the GCs in M31. I will also briefly mention the effects of multiple populations on IL spectra, and how observations of distant globular clusters help constrain the source(s) of light-element abundance variations. I will end with future perspectives, emphasizing how IL spectroscopy can bridge the gap between Galactic and extragalactic astronomy.

Keywords

Globular clusterschemical abundanceschemical evolution
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. 155 - 160
Copyright
© International Astronomical Union 2020

Footnotes

†

Present address: Department of Physics & Astronomy, San Francisco State University, 1600 Holloway Avenue, San Francisco, CA 94132.

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