Looze, ID;
Lamperti, I;
Saintonge, A;
Relano, M;
Smith, MWL;
Clark, CJR;
Wilson, CD;
... Zhu, M; + view all
(2020)
JINGLE -- IV. Dust, HI gas and metal scaling laws in the local Universe.
Monthly Notices of the Royal Astronomical Society,3668–3687
, 496
(3)
pp. 3668-3687.
10.1093/mnras/staa1496.
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Abstract
Scaling laws of dust, H I gas, and metal mass with stellar mass, specific star formation rate, and metallicity are crucial to our understanding of the build-up of galaxies through their enrichment with metals and dust. In this work, we analyse how the dust and metal content varies with specific gas mass (MH I/M⋆) across a diverse sample of 423 nearby galaxies. The observed trends are interpreted with a set of Dust and Element evolUtion modelS (DEUS) – including stellar dust production, grain growth, and dust destruction – within a Bayesian framework to enable a rigorous search of the multidimensional parameter space. We find that these scaling laws for galaxies with −1.0 ≲ log MH I/M⋆ ≲ 0 can be reproduced using closed-box models with high fractions (37–89 per cent) of supernova dust surviving a reverse shock, relatively low grain growth efficiencies (ϵ = 30–40), and long dust lifetimes (1–2 Gyr). The models have present-day dust masses with similar contributions from stellar sources (50–80 per cent) and grain growth (20–50 per cent). Over the entire lifetime of these galaxies, the contribution from stardust (>90 per cent) outweighs the fraction of dust grown in the interstellar medium (<10 per cent). Our results provide an alternative for the chemical evolution models that require extremely low supernova dust production efficiencies and short grain growth time-scales to reproduce local scaling laws, and could help solving the conundrum on whether or not grains can grow efficiently in the interstellar medium.
Type: | Article |
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Title: | JINGLE -- IV. Dust, HI gas and metal scaling laws in the local Universe |
Open access status: | An open access version is available from UCL Discovery |
DOI: | 10.1093/mnras/staa1496 |
Publisher version: | http://dx.doi.org/10.1093/mnras/staa1496 |
Language: | English |
Additional information: | This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions. |
Keywords: | ISM: abundances, ISM: dust, extinction, galaxies: evolution, galaxies: star formation |
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/10101285 |
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