Age as a major factor in the onset of multiple populations in stellar clusters
Abstract. It is now well established that globular clusters (GCs) exhibit star-to-star light-element abundance variations (known as multiple populations, MPs).
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 473, Heft: 2, Pages: 2688-2700 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stx2556 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1093/mnras/stx2556 Verlag, Volltext: https://academic.oup.com/mnras/article/473/2/2688/4315957 
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| Verfasserangaben: | S. Martocchia, I. Cabrera-Ziri, C. Lardo, E. Dalessandro, N. Bastian, V. Kozhurina-Platais, C. Usher, F. Niederhofer, M. Cordero, D. Geisler, K. Hollyhead, N. Kacharov, S. Larsen, C. Li, D. Mackey, M. Hilker, A. Mucciarelli, I. Platais and M. Salaris |
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| 520 | |a Abstract. It is now well established that globular clusters (GCs) exhibit star-to-star light-element abundance variations (known as multiple populations, MPs). | ||
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