Tracing the total molecular gas in galaxies: [CII] and the CO-dark gas
Tracing the total molecular gas in galaxies: [CII] and the CO-dark gas
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Author / Creator
Madden, S C , Cormier, D , Hony, S , Lebouteiller, V , Abel, N , Galametz, M , De Looze, I , Chevance, M , Polles, F L , M -Y Lee , Galliano, F , Lambert-Huyghe, A , D Hu and Ramambason, L
Publisher
Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
While the CO(1-0) transition is often used to deduce the total molecular hydrogen in galaxies, it is challenging to detect in low metallicity galaxies, in spite of the star formation taking place. In contrast, the [CII] 158 micron line is relatively bright, highlighting a potentially important reservoir of H2 that is not traced by CO(1-0), but resi...
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Full title
Tracing the total molecular gas in galaxies: [CII] and the CO-dark gas
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TN_cdi_proquest_journals_2439762211
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2439762211
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2009.00649
