Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback
Observations that molecular gas in NGC 300 is spatially uncorrelated with high-mass stars are attributed to rapid evolution, with molecular clouds quickly destroyed by stellar feedback, and low star-formation efficiency.
Gespeichert in:
| Hauptverfasser: | , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
22 May 2019
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| In: |
Nature
Year: 2019, Jahrgang: 569, Heft: 7757, Pages: 519-538 |
| ISSN: | 1476-4687 |
| DOI: | 10.1038/s41586-019-1194-3 |
| Online-Zugang: | Verlag, Volltext: https://doi.org/10.1038/s41586-019-1194-3 Verlag, Volltext: https://www.nature.com/articles/s41586-019-1194-3 
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| Verfasserangaben: | J.M. Diederik Kruijssen, Andreas Schruba, Mélanie Chevance, Steven N. Longmore, Alexander P.S. Hygate, Daniel T. Haydon, Anna F. McLeod, Julianne J. Dalcanton, Linda J. Tacconi & Ewine F. van Dishoeck |
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| 520 | |a Observations that molecular gas in NGC 300 is spatially uncorrelated with high-mass stars are attributed to rapid evolution, with molecular clouds quickly destroyed by stellar feedback, and low star-formation efficiency. | ||
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