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
Saved in:
| Main Authors: | , |
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| Format: | Article (Journal) |
| Language: | English |
| Published: |
06 March 2012
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2012, Volume: 421, Issue: 1, Pages: 9-19 |
| ISSN: | 1365-2966 |
| DOI: | 10.1111/j.1365-2966.2011.19648.x |
| Online Access: | 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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| Author Notes: | Simon C.O. Glover and Paul C. Clark |
| Summary: | 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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| Item Description: | Gesehen am 31.08.2018 |
| Physical Description: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1111/j.1365-2966.2011.19648.x |