Comparing young massive clusters and their progenitor clouds in the Milky Way
Young massive clusters (YMCs) have central stellar mass surface densities exceeding 104 M⊙ pc−2. It is currently unknown whether the stars formed at such high (proto)stellar densities. We compile a sample of gas clouds in the Galaxy which have sufficient gas mass within a radius of a few parsecs to...
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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
10 February 2016
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2016, Jahrgang: 457, Heft: 4, Pages: 4536-4545 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stw313 |
| Online-Zugang: | Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stw313
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| Verfasserangaben: | D.L. Walker, S.N. Longmore, N. Bastian, J.M.D. Kruijssen, J.M. Rathborne, R. Galván-Madrid and H.B. Liu |
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Comparing young massive clusters and their progenitor clouds in the Milky Way
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