The DOI matches its Crossref record; 336 of the 336 references it cites were found in a registry or an index.
Multiple populations in globular clusters: Lessons learned from the Milky Way globular clusters
Open accessAbstract
Recent progress in studies of globular clusters has shown that they are not simple stellar populations, but rather are made up of multiple generations. Evidence stems both from photometry and spectroscopy. A new paradigm is arising for the formation of massive star clusters, which includes several episodes of star formation. While this provides an explanation for several features of globular clusters, including the second-parameter problem, it also opens new perspectives on the relation between globular clusters and the halo of our Galaxy, and by extension on all populations with a high specific frequency of globular clusters, such as, e.g., giant elliptical galaxies. We review progress in this area, focussing on the most recent studies. Several points remain to become properly understood, in particular those concerning the nature of the polluters producing the abundance pattern in the clusters and the typical timescale, the range of cluster masses where this phenomenon is active, and the relation between globular clusters and other satellites of our Galaxy.
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Cited by
MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS
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The Apache Point Observatory Galactic Evolution Experiment (APOGEE)
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The dragon simulations: globular cluster evolution with a million stars
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Metadata
- Authors
- Gratton, R. G., Carretta, E., & Bragaglia, A.
- Venue
- The Astronomy and Astrophysics Review
- Published
- 2012-02-28
- Volume
- 20
- Issue
- 1
- ISSN
- 0935-4956 (ISSN-L)
- 1432-0754
- OpenAlex
- W3125024839
- Cited by
- 787
- References
- 336
- FWCI
- 46.07
- Type
- journal article
- Language
- en
- Open access
- green
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