M.T. Huynh
Detection of molecular gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44
Huynh, M.T.; Kimball, A.E.; Norris, R.P.; Smail, I.; Chow, K.E.; Coppin, K.E.K.; Emonts, B.H.C.; Ivison, R.J.; Smolčić, V.; Swinbank, A.M.
Authors
A.E. Kimball
R.P. Norris
Ian Smail ian.smail@durham.ac.uk
Emeritus Professor
K.E. Chow
K.E.K. Coppin
B.H.C. Emonts
R.J. Ivison
V. Smolčić
Professor Mark Swinbank a.m.swinbank@durham.ac.uk
Professor
Abstract
We present the detection of 12CO(2–1) in the z = 4.44 submillimetre galaxy ALESS65.1 using the Australia Telescope Compact Array. A previous Atacama Large Millimeter/submillimeter Array study of submillimetre galaxies (SMGs) in the Extended Chandra Deep Field South determined the redshift of this optically and near-infrared undetected source through the measurement of [C II] 157.74 μm emission. Using the luminosity of the 12CO(2–1) emission, we estimate the gas mass to be Mgas ∼ 1.7 × 1010 M⊙. The gas depletion time-scale of ALESS65.1 is ∼ 25 Myr, similar to other high-redshift SMGs and consistent with z > 4 SMGs being the progenitors of massive ‘red-and-dead’ galaxies at z > 2. The ratio of the [C II], 12CO and far-infrared luminosities implies a strong far-ultraviolet field of G0 ∼ 103.25, which is at the high end of the far-ultraviolet fields seen in local starbursts, but weaker than the far-ultraviolet fields of most nearby ultraluminous infrared galaxies (ULIRGs). The high ratio of L[CII]/LFIR=1.0×10−3 observed in ALESS65.1, combined with L[CII]/LCO∼2300, is consistent with ALESS65.1 having more extended regions of intense star formation than local ULIRGs.
Citation
Huynh, M., Kimball, A., Norris, R., Smail, I., Chow, K., Coppin, K., …Swinbank, A. (2014). Detection of molecular gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44. Monthly Notices of the Royal Astronomical Society: Letters, 443(1), L54-L58. https://doi.org/10.1093/mnrasl/slu077
Journal Article Type | Article |
---|---|
Publication Date | Sep 1, 2014 |
Deposit Date | Nov 17, 2014 |
Publicly Available Date | Nov 24, 2014 |
Journal | Monthly Notices of the Royal Astronomical Society: Letters |
Electronic ISSN | 1745-3933 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 443 |
Issue | 1 |
Pages | L54-L58 |
DOI | https://doi.org/10.1093/mnrasl/slu077 |
Keywords | galaxies: evolution, Galaxies: formation, Radio lines: galaxies |
Public URL | https://durham-repository.worktribe.com/output/1441965 |
Files
Published Journal Article
(330 Kb)
PDF
Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society: Letters © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society All rights reserved.
You might also like
3D tomography of the giant Lyα nebulae of z ≈ 3–5 radio-loud AGN
(2023)
Journal Article
Downloadable Citations
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2024
Advanced Search