Star formation in metal-poor gas clouds
Abstract. Observations of molecular clouds in metal-poor environments typically find that they have much higher star formation rates than one would expect base
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
11 October 2012
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2012, Jahrgang: 426, Heft: 1, Pages: 377-388 |
| ISSN: | 1365-2966 |
| DOI: | 10.1111/j.1365-2966.2012.21737.x |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1111/j.1365-2966.2012.21737.x Verlag, Volltext: https://academic.oup.com/mnras/article/426/1/377/1008432 
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| Verfasserangaben: | Simon C.O. Glover and Paul C. Clark |
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