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A multiwavelength exploration of the [C II]/IR ratio in H-ATLAS/GAMA galaxies out to z = 0.2
Journal article published in 2015 by
E. Ibar,
M. A. Lara-Lopez 
,
R. Herrera-Camus,
R. Hopwood,
A. Bauer,
R. J. Ivison,
M. J. Michalowski,
M. J. Micha owski,
H. Dannerbauer,
P. van der Werf,
D. Riechers,
N. Bourne,
M. Baes ,
I. Valtchanov,
Loretta Dunne
and other authors.
,
R. Herrera-Camus,
R. Hopwood,
A. Bauer,
R. J. Ivison,
M. J. Michalowski,
M. J. Micha owski,
H. Dannerbauer,
P. van der Werf,
D. Riechers,
N. Bourne,
M. Baes ,
I. Valtchanov,
Loretta Dunne
and other authors.
Abstract
We explore the behaviour of [C II] λ157.74 μm forbidden fine-structure line observed in a sample of 28 galaxies selected from ∼ 50 deg 2 of the Herschel-Astrophysical Terahertz Large Area Survey survey. The sample is restricted to galaxies with flux densities higher than S 160μm > 150 mJy and optical spectra from the Galaxy and Mass Assembly survey at 0.02 2.5×10 −3 with respect to those showing lower ratios. In particular, those with high ratios tend to have: (1) L IR