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JINGLE -- IV. Dust, HI gas and metal scaling laws in the local Universe

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. Green open access

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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
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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