Dynamical cluster disruption and its implications for multiple population models in the E-MOSAICS simulations
ABSTRACT. Several models have been advanced to explain the multiple stellar populations observed in globular clusters (GCs). Most models necessitate a large in
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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018 September 10
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 481, Heft: 3, Pages: 2851-2857 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty2451 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2451 Verlag, Volltext: https://academic.oup.com/mnras/article/481/3/2851/5094599 
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| Verfasserangaben: | M. Reina-Campos, J.M.D. Kruijssen, J. Pfeffer, N. Bastian and R.A. Crain |
| Zusammenfassung: | ABSTRACT. Several models have been advanced to explain the multiple stellar populations observed in globular clusters (GCs). Most models necessitate a large in |
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| Beschreibung: | Gesehen am 24.01.2019 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty2451 |