Is molecular gas necessary for star formation?
Abstract. On galactic scales, the surface density of star formation appears to be well correlated with the surface density of molecular gas. This has led many
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
06 March 2012
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2012, Jahrgang: 421, Heft: 1, Pages: 9-19 |
| ISSN: | 1365-2966 |
| DOI: | 10.1111/j.1365-2966.2011.19648.x |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1111/j.1365-2966.2011.19648.x Verlag, Volltext: https://academic.oup.com/mnras/article/421/1/9/989344 
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| Verfasserangaben: | Simon C.O. Glover and Paul C. Clark |
| Zusammenfassung: | Abstract. On galactic scales, the surface density of star formation appears to be well correlated with the surface density of molecular gas. This has led many |
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| Beschreibung: | Gesehen am 31.08.2018 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1111/j.1365-2966.2011.19648.x |