Young massive star cluster formation in the Galactic Centre is driven by global gravitational collapse of high-mass molecular clouds
Abstract. Young massive clusters (YMCs) are the most compact, high-mass stellar systems still forming at the present day. The precursor clouds to such systems
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2019 March 19
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2019, Jahrgang: 486, Heft: 1, Pages: 283-303 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stz796 |
| Online-Zugang: | Verlag, Volltext: https://doi.org/10.1093/mnras/stz796 Verlag, Volltext: https://academic.oup.com/mnras/article/486/1/283/5393403 
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| Verfasserangaben: | A.T. Barnes, S.N. Longmore, A. Avison, Y. Contreras, A. Ginsburg, J.D. Henshaw, J.M. Rathborne, D.L. Walker, J. Alves, J. Bally, C. Battersby, M.T. Beltrán, H. Beuther, G. Garay, L. Gomez, J. Jackson, J. Kainulainen, J.M.D. Kruijssen, X. Lu, E.a.C. Mills, J. Ott and T. Peters |
| Zusammenfassung: | Abstract. Young massive clusters (YMCs) are the most compact, high-mass stellar systems still forming at the present day. The precursor clouds to such systems |
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| Beschreibung: | Gesehen am 31.05.2019 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stz796 |