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Thirteen facts that you need to know on multiple populations in globular clusters

Published online by Cambridge University Press:  11 March 2020

Antonino P. Milone Open the ORCID record for Antonino P. Milone [Opens in a new window]
Antonino P. Milone*
Affiliation:
Dipartimento di Fisica e Astronomia “Galileo Galilei”, Univ. di Padova, Vicolo dell’Osservatorio 3, Padova, IT-35122 email: antonino.milone@unipd.it
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Abstract

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I review the methods, mostly developed in the last decade, that are commonly used to identify and characterize multiple populations (MPs) in Globular Clusters (GCs) based on photometry. I summarize the results from the recent surveys of MPs with the Hubble Space Telescope (HST) and ground-based facilities and provide a list of the main properties of MPs as inferred from these studies.

Keywords

stars: Population IIstars: abundances(Galaxy:) globular clusters: generalGalaxy: halo(galaxies:) Magellanic Clouds
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. 251 - 260
Copyright
© International Astronomical Union 2020

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