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Publication Details
AFRICAN RESEARCH NEXUS
SHINING A SPOTLIGHT ON AFRICAN RESEARCH
earth and planetary sciences
A multiwavelength exploration of the [C II]/IR ratio in H-ATLAS/GAMA galaxies out to z = 0.2
Monthly Notices of the Royal Astronomical Society, Volume 449, No. 3, Year 2015
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Description
We explore the behaviour of [C II] λ157.74 μm forbidden fine-structure line observed in a sample of 28 galaxies selected from ~ 50 deg2 of the Herschel-Astrophysical Terahertz Large Area Survey survey. The sample is restricted to galaxies with flux densities higher than S160μm > 150 mJy and optical spectra from the Galaxy and Mass Assembly survey at 0.02 < z < 0.2. Far-IR spectra centred on this redshifted line were taken with the Photodetector Array Camera and Spectrometer instrument on-board the Herschel Space Observatory. The galaxies span 10 < log(LIR/L⊙) < 12 (where LIR ≡ LIR[8-1000 μm]) and 7.3 < log(L[C II]/L⊙) < 9.3, covering a variety of optical galaxy morphologies. The sample exhibits the so-called [CII] deficit at high-IR luminosities, i.e. L[C II]/LIR (hereafter [CII]/IR) decreases at high LIR. We find significant differences between those galaxies presenting [C II]/IR > 2.5×10-3 with respect to those showing lower ratios. In particular, those with high ratios tend to have: (1) LIR < 1011 L⊙; (2) cold dust temperatures, Td < 30 K; (3) disc-like morphologies in r-band images; (4) a Wide-field Infrared Survey Explorer colour 0.5 ≲ S12μm/S22μm ≲ 1.0; (5) low surface brightness ΣIR ≈108-9 L⊙ kpc-2, (6) and specific star formation rates of sSFR ≈0.05-3 Gyr-1. We suggest that the strength of the far-UV radiation fields (〈GO〉) is main parameter responsible for controlling the [C II]/IR ratio. It is possible that relatively high 〈GO〉 creates a positively charged dust grain distribution, impeding an efficient photoelectric extraction of electrons from these grains to then collisionally excite carbon atoms. Within the brighter IR population, 11 < log(LIR/L⊙) < 12, the low [C II]/IR ratio is unlikely to be modified by [C II] self-absorption or controlled by the presence of a moderately luminous AGN (identified via the BPT diagram). © 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.
Authors & Co-Authors
Ibar, E.
Chile, Valparaiso
Universidad de Valparaiso
Lara-López, Maritza A.
Mexico, Mexico
Universidad Nacional Autónoma de México
Australia
Australian Astronomical Observatory
Herrera-Camus, Rodrigo
United States, College Park
University of Maryland, College Park
Hopwood, Rosalind H.B.
United Kingdom, London
Imperial College London
Bauer, Amanda E.
Australia
Australian Astronomical Observatory
Ivison, Robert J.
Germany, Garching Bei Munchen
European Southern Observatory
United Kingdom, Edinburgh
The University of Edinburgh
Michałowski, Michał J.
United Kingdom, Edinburgh
The University of Edinburgh
Dannerbauer, Helmut
Austria, Vienna
Universität Wien
van der Werf, Paul P.
Netherlands, Leiden
Universiteit Leiden
Riechers, Dominick A.
United States, Pasadena
California Institute of Technology
United States, Ithaca
Cornell University
Bourne, Nathan
United Kingdom, Edinburgh
The University of Edinburgh
Baes, Maarten
Belgium, Ghent
Universiteit Gent
Valtchanov, Ivan
Spain, Madrid
European Space Astronomy Centre
Dunne, Loretta
United Kingdom, Edinburgh
The University of Edinburgh
New Zealand, Christchurch
University of Canterbury
Verma, Aprajita
United Kingdom, Oxford
University of Oxford
Brough, Sarah
Australia
Australian Astronomical Observatory
Cooray, Asantha Roshan
United States, Pasadena
California Institute of Technology
United States, Irvine
University of California, Irvine
de Zotti, Gianfranco
Italy, Rome
Istituto Nazionale Di Astrofisica, Rome
Italy, Trieste
Scuola Internazionale Superiore Di Studi Avanzati
Dye, S.
United Kingdom, Nottingham
University of Nottingham
Eales, Stephen A.
United Kingdom, Cardiff
Cardiff University
Furlanetto, C.
United Kingdom, Nottingham
University of Nottingham
Brazil, Brasilia
Ministry of Education Brazil
Maddox, Steve J.
United Kingdom, Edinburgh
The University of Edinburgh
New Zealand, Christchurch
University of Canterbury
Smith, Matthew W.L.
United Kingdom, Cardiff
Cardiff University
Steele, Oliver I.
United Kingdom, Portsmouth
University of Portsmouth
Thomas, Daniel B.
United Kingdom, Portsmouth
University of Portsmouth
Valiante, Elisabetta
United Kingdom, Cardiff
Cardiff University
Statistics
Citations: 24
Authors: 26
Affiliations: 22
Identifiers
Doi:
10.1093/mnras/stv439
ISSN:
00358711
Research Areas
Cancer
Environmental
Study Design
Cross Sectional Study
Study Approach
Quantitative