Does the CO-to-H2 conversion factor depend on the star formation rate?
Abstract. We present a series of numerical simulations that explore how the ‘X-factor’, XCO - the conversion factor between the observed integrated CO emission
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
21 July 2015
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2015, Jahrgang: 452, Heft: 2, Pages: 2057-2070 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stv1369 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stv1369 Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/452/2/2057/1061966 
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| Verfasserangaben: | Paul C. Clark, Simon C. O. Glover |
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