The DOI matches its Crossref record; 246 of the 246 references it cites were found in a registry or an index.
Multiple Stellar Populations in Globular Clusters
Open accessAbstract
Globular clusters (GCs) exhibit star-to-star variations in specific elements (e.g., He, C, N, O, Na, Al) that bear the hallmark of high-temperature H-burning. These abundance variations can be observed spectroscopically and also photometrically, with the appropriate choice of filters, due to the changing of spectral features within the band pass. This phenomenon is observed in nearly all of the ancient GCs, although, to date, it has not been found in any massive cluster younger than 2 Gyr. Many scenarios have been suggested to explain this phenomenon, with most invoking multiple epochs of star formation within the cluster; however, all have failed to reproduce various key observations, in particular when a global view of the GC population is taken. We review the state of current observations and outline the successes and failures of each of the main proposed models. The traditional idea of using the stellar ejecta from a first generation of stars to form a second generation of stars, while conceptually straightforward, has failed to reproduce an increasing number of observational constraints. We conclude that the puzzle of multiple populations remains unsolved, hence alternative theories are needed.
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Cites
A Catalog of Parameters for Globular Clusters in the Milky Way
Harris, W. E. (1996) · The Astronomical Journal · doi:10.1086/118116 · Cited by 4,500
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Abundance Variations within Globular Clusters
Gratton, R., Sneden, C., & Carretta, E. (2004) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.42.053102.133945 · Cited by 885
Carretta, E., Bragaglia, A., Gratton, R. G., Lucatello, S., Catanzaro, G., Leone, F., Bellazzini, M., Claudi, R., D'Orazi, V., Momany, Y., et al. (2009) · Astronomy & Astrophysics · doi:10.1051/0004-6361/200912096 · Cited by 856
Multiple populations in globular clusters: Lessons learned from the Milky Way globular clusters
Gratton, R. G., Carretta, E., & Bragaglia, A. (2012) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-012-0050-3 · Cited by 787
The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars
Karakas, A. I., & Lattanzio, J. C. (2014) · Publications of the Astronomical Society of Australia · doi:10.1017/pasa.2014.21 · Cited by 735
Fast rotating massive stars and the origin of the abundance patterns in galactic globular clusters
Decressin, T., Meynet, G., Charbonnel, C., Prantzos, N., & Ekström, S. (2007) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20066013 · Cited by 690
A Triple Main Sequence in the Globular Cluster NGC 2808
Piotto, G., Bedin, L. R., Anderson, J., King, I. R., Cassisi, S., Milone, A. P., Villanova, S., Pietrinferni, A., & Renzini, A. (2007) · The Astrophysical Journal · doi:10.1086/518503 · Cited by 689
Formation and dynamical evolution of multiple stellar generations in globular clusters
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Cited by
Evidence from the H3 Survey That the Stellar Halo Is Entirely Comprised of Substructure
Naidu, R. P., Conroy, C., Bonaca, A., Johnson, B. D., Ting 丁, Y.-S. 源., Caldwell, N., Zaritsky, D., & Cargile, P. A. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/abaef4 · Cited by 389
The formation and assembly history of the Milky Way revealed by its globular cluster population
Kruijssen, J. M. D., Pfeffer, J. L., Reina-Campos, M., Crain, R. A., & Bastian, N. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sty1609 · Cited by 369
Self-citation
Metadata
- Authors
- Bastian, N., & Lardo, C.
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 2018-09-14
- Volume
- 56
- Issue
- 1
- Pages
- 83-136
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2775727542
- Cited by
- 685
- References
- 246
- FWCI
- 9.42
- Type
- journal article
- Language
- en
- Open access
- bronze
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Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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