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
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| Hauptverfasser: | , |
|---|---|
| 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 |
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