1. The ALMA REBELS survey: the dust content of z~7 Lyman break galaxies
- Author
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P Dayal, A Ferrara, L Sommovigo, R Bouwens, P A Oesch, R Smit, V Gonzalez, S Schouws, M Stefanon, C Kobayashi, J Bremer, H S B Algera, M Aravena, R A A Bowler, E da Cunha, Y Fudamoto, L Graziani, J Hodge, H Inami, I De Looze, A Pallottini, D Riechers, R Schneider, D Stark, R Endsley, Astronomy, Dayal, P., Ferrara, A., Sommovigo, L., Bouwens, R., Oesch, P. A., Smit, R., Gonzalez, V., Schouws, S., Stefanon, M., Kobayashi, C., Bremer, J., Algera, H. S. B., Aravena, M., Bowler, R. A. A., Da Cunha, E., Fudamoto, Y., Graziani, L., Hodge, J., Inami, H., De Looze, I., Pallottini, A., Riechers, D., Schneider, R., Stark, D., and Endsley, R.
- Subjects
dust ,extinction ,galaxies: evolution ,galaxies: high-redshift ,galaxies: ISM ,galaxies: luminosity function ,mass function ,Astrophysics - Astrophysics of Galaxies ,1ST BILLION YEARS ,Astrophysics - astrophysics of galaxies ,FOS: Physical sciences ,Astrophysics::Cosmology and Extragalactic Astrophysics ,MASS ,STAR-FORMATION ,Settore FIS/05 - Astronomia e Astrofisica ,Astrophysics::Solar and Stellar Astrophysics ,Galaxies - ISM ,QC ,evolution [galaxies] ,Astrophysics::Galaxy Astrophysics ,Galaxies - high-redshift ,QB ,EPOCH ,ISM [galaxies] ,UV-CONTINUUM SLOPE ,Galaxies - evolution ,Astronomy and Astrophysics ,Dust ,Extinction ,Galaxies - luminosity function ,luminosity function, mass function [galaxies] ,EVOLUTION ,Physics and Astronomy ,Space and Planetary Science ,ULTRA-DEEP FIELD ,LUMINOSITY FUNCTION ,Astrophysics of Galaxies (astro-ph.GA) ,Mass function ,dust, extinction ,Astrophysics::Earth and Planetary Astrophysics ,HIGH-REDSHIFT ,high-redshift [galaxies] ,INTERSTELLAR DUST - Abstract
We include a fully coupled treatment of metal and dust enrichment into the Delphi semi-analytic model of galaxy formation to explain the dust content of 13 Lyman Break Galaxies (LBGs) detected by the Atacama Large millimetre Array (ALMA) REBELS Large Program at $z\simeq 7$. We find that the galaxy dust mass, $M_d$, is regulated by the combination of SNII dust production, astration, shock destruction, and ejection in outflows; grain growth (with a standard timescale $\tau_0= 30$ Myr) plays a negligible role. The model predicts a dust-to-stellar mass ratio of $\sim 0.07-0.1\%$ and a UV-to-total star formation rate relation such that $log (\psi_{\rm UV}) = -0.05 ~[log (\psi)]^{2} + 0.86 ~log(\psi) -0.05$ (implying that 55-80\% of the star formation is obscured) for REBELS galaxies with stellar mass $M_* = 10^{9-10} M_\odot$. This relation reconciles the intrinsic UV luminosity of LBGs with their observed luminosity function at $z=7$. However, 2 out of the 13 systems show dust-to-stellar mass ratios ($\sim 0.94-1.1\%$) that are up to $18\times$ larger than expected from the fiducial relation. Due to the physical coupling between dust and metal enrichment, even decreasing $\tau_0$ to very low values (0.3 Myr) only increases the dust-to-stellar mass ratio by a factor $ \sim 2$. Given that grain growth is not a viable explanation for such high observed ratios of the dust-to-stellar mass, we propose alternative solutions., Comment: Accepted to MNRAS
- Published
- 2022
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