The CO-dark molecular gas mass in 30 Doradus
ABSTRACT. Determining the efficiency with which gas is converted into stars in galaxies requires an accurate determination of the total reservoir of molecular
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| Hauptverfasser: | , , , , , , , , , , , , , , , , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
23 April 2020
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2020, Jahrgang: 494, Heft: 4, Pages: 5279-5292 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/staa1106 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/staa1106 Verlag, lizenzpflichtig, Volltext: https://academic.oup.com/mnras/article/494/4/5279/5824169 
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| Verfasserangaben: | Mélanie Chevance, Suzanne C. Madden, Christian Fischer, William D. Vacca, Vianney Lebouteiller, Dario Fadda, Frédéric Galliano, Remy Indebetouw, J. M. Diederik Kruijssen, Min-Young Lee, Albrecht Poglitsch, Fiorella L. Polles, Diane Cormier, Sacha Hony, Christof Iserlohe, Alfred Krabbe, Margaret Meixner, Elena Sabbi and Hans Zinnecker |
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