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- W2581494544 abstract "Galactic globular clusters are not simple stellar populations. And nothing is simple in their study, basically because we try to reconstruct chains of events that occurred at redshift z > 2-3 by observing these objects at z=0, after a Hubble time. Fortunately, spectroscopy offers a magnifying lens: differences of tens or hundreds of Myrs between stellar generations are translated into differences in abundances up to a full dex. I will review the complex pattern emerging by the combined efforts of different groups, focusing on the chemical signatures of multiple populations in globular clusters." @default.
- W2581494544 created "2017-02-03" @default.
- W2581494544 creator A5084788706 @default.
- W2581494544 date "2016-11-15" @default.
- W2581494544 modified "2023-09-27" @default.
- W2581494544 title "Spectroscopic evidence of Multiple Stellar Populations in Globular Clusters" @default.
- W2581494544 hasPublicationYear "2016" @default.
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