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xGASS: Total cold gas scaling relations and molecular-to-atomic gas ratios of galaxies in the local Universe

Catinella, B; Saintonge, A; Janowiecki, S; Cortese, L; Davé, R; Lemonias, JJ; Cooper, AP; ... Wang, J; + view all (2018) xGASS: Total cold gas scaling relations and molecular-to-atomic gas ratios of galaxies in the local Universe. Monthly Notices of the Royal Astronomical Society , 476 (1) pp. 875-895. 10.1093/mnras/sty089. Green open access

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Abstract

We present the extended GALEX Arecibo SDSS Survey (xGASS), a gas fraction-limited censusof the atomic hydrogen (H I) gas content of 1179 galaxies selected only by stellar mass (M* = 10 9 - 1011.5 Mo˙) and redshift (0.01 < z < 0.05). This includes new Arecibo observations of 208galaxies, for which we release catalogues and HI spectra. In addition to extending the GASSHI scaling relations by one decade in stellar mass, we quantify total (atomic+molecular) coldgas fractions and molecular-to-atomic gas mass ratios, R mol , for the subset of 477 galaxiesobserved with the IRAM 30 m telescope. We find that atomic gas fractions keep increasingwith decreasing stellar mass, with no sign of a plateau down to logM*/Mo˙ = 9. Total gasreservoirs remain HI-dominated across our full stellar mass range, hence total gas fractionscaling relations closely resemble atomic ones, but with a scatter that strongly correlates withR mol , especially at fixed specific star formation rate. On average, R mol weakly increases withstellar mass and stellar surface density μ*, but individual values vary by almost two ordersof magnitude at fixed M* or μ*. We show that, for galaxies on the star-forming sequence, variations of R mol are mostly driven by changes of the HI reservoirs, with a clear dependenceon μ*. Establishing if galaxy mass or structure plays the most important role in regulating thecold gas content of galaxies requires an accurate separation of bulge and disc components forthe study of gas scaling relations.

Type: Article
Title: xGASS: Total cold gas scaling relations and molecular-to-atomic gas ratios of galaxies in the local Universe
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/sty089
Publisher version: https://doi.org/10.1093/mnras/sty089
Language: English
Additional information: This is the published version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: galaxies: evolution, galaxies: fundamental parameters, galaxies: ISM, radio lines: galaxies
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10046206
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