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
Saved in:
| Main Authors: | , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
21 July 2015
|
| In: |
Monthly notices of the Royal Astronomical Society
Year: 2015, Volume: 452, Issue: 2, Pages: 2057-2070 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stv1369 |
| Online Access: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stv1369 Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/452/2/2057/1061966 
|
| Author Notes: | Paul C. Clark, Simon C. O. Glover |
| Summary: | Abstract. We present a series of numerical simulations that explore how the ‘X-factor’, XCO - the conversion factor between the observed integrated CO emission |
|---|---|
| Item Description: | Gesehen am 01.12.2020 |
| Physical Description: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stv1369 |