The dynamical origin of multiple populations in intermediate-age clusters in the Magellanic Clouds
Numerical simulations were carried out to study the origin of multiple stellar populations in the intermediate-age clusters NGC 411 and NGC 1806 in the Magellanic Clouds. We performed nbody6++ simulations based on two different formation scenarios, an ad hoc formation model where second-generation (...
Gespeichert in:
| Hauptverfasser: | , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2017 July 2
|
| In: |
Monthly notices of the Royal Astronomical Society
Year: 2017, Jahrgang: 472, Heft: 1, Pages: 67-77 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stx1954 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx1954
|
| Verfasserangaben: | Jongsuk Hong, Richard de Grijs, Abbas Askar, Peter Berczik, Chengyuan Li, Long Wang, Licai Deng, M.B.N. Kouwenhoven, Mirek Giersz and Rainer Spurzem |
Search Result 1
The dynamical origin of multiple populations in intermediate-age clusters in the magellanic clouds
Article (Journal)
Kapitel/Artikel
Online Resource