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The dust budget crisis in high-redshift submillimetre galaxies

Rowlands, K.; Gomez, H.L.; Dunne, L.; Aragón-Salamanca, Alfonso; Dye, S.; Maddox, S.; da Cunha, E.; van der Werf, Paul

Authors

K. Rowlands

H.L. Gomez

L. Dunne

SIMON DYE Simon.Dye@nottingham.ac.uk
Associate Professor

S. Maddox

E. da Cunha

Paul van der Werf



Abstract

We apply a chemical evolution model to investigate the sources and evolution of dust in a sample of 26 high-redshift (z > 1) submillimetre galaxies (SMGs) from the literature, with complete photometry from ultraviolet to the submillimetre. We show that dust produced only by low–intermediate-mass stars falls a factor 240 short of the observed dust masses of SMGs, the well-known ‘dust-budget crisis’. Adding an extra source of dust from supernovae can account for the dust mass in 19 per cent of the SMG sample. Even after accounting for dust produced by supernovae the remaining deficit in the dust mass budget provides support for higher supernova yields, substantial grain growth in the interstellar medium or a top-heavy IMF. Including efficient destruction of dust by supernova shocks increases the tension between our model and observed SMG dust masses. The models which best reproduce the physical properties of SMGs have a rapid build-up of dust from both stellar and interstellar sources and minimal dust destruction. Alternatively, invoking a top-heavy IMF or significant changes in the dust grain properties can solve the dust budget crisis only if dust is produced by both low-mass stars and supernovae and is not efficiently destroyed by supernova shocks.

Citation

Rowlands, K., Gomez, H., Dunne, L., Aragón-Salamanca, A., Dye, S., Maddox, S., …van der Werf, P. (in press). The dust budget crisis in high-redshift submillimetre galaxies. Monthly Notices of the Royal Astronomical Society, 441(2), https://doi.org/10.1093/mnras/stu605

Journal Article Type Article
Acceptance Date Mar 26, 2014
Online Publication Date May 5, 2014
Deposit Date Jul 11, 2016
Publicly Available Date Jul 11, 2016
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 441
Issue 2
DOI https://doi.org/10.1093/mnras/stu605
Keywords dust, extinction; ISM: evolution; galaxies: evolution; galaxies: high redshift; submillimetre: galaxies.
Public URL http://eprints.nottingham.ac.uk/id/eprint/34794
Publisher URL https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stu605
Copyright Statement Copyright information regarding this work can be found at the following address: http://eprints.nottingh.../end_user_agreement.pdf
Additional Information This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2014 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

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Copyright Statement
Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf





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