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Huynh, M. T; Norris, R. P; Coppin, K. E. K; Emonts, B. H. C; Ivison, R. J; Seymour, N; Smail, Ian; Smol i, V; Swinbank, A. M; Brandt, W. N; Chapman, S. C; Dannerbauer, H; De Breuck, C; Greve, T. R; Hodge, J. A; Karim, A; Knudsen, K. K; Menten, K. M; van der Werf, P. P; Walter, F; Weiss, A
Monthly notices of the Royal Astronomical Society. Letters, 05/2013, Volume: 431, Issue: 1Journal Article
We present 12CO(2-1) observations of the submillimetre galaxy ALESS65.1 performed with the Australia Telescope Compact Array (ATCA) at 42.3 GHz. A previous Atacama Large Millimeter Array study of submillimetre galaxies (SMGs) in the Extended Chandra Deep Field South detected C ii 157.74 μm emission from this galaxy at a redshift of z = 4.44. No 12CO(2-1) emission was detected but we derive a firm upper limit to the cold gas mass in ALESS65.1 of . The estimated gas depletion time-scale is <50 Myr, which is similar to other high-redshift SMGs, and consistent with z > 4 SMGs being the likely 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 G 0 103, as seen in Galactic star-forming regions or local ultraluminous infrared galaxies (ULIRGs). The observed is high compared to local ULIRGs and, combined with , it is consistent with ALESS65.1 either having an extended (several kpc) C ii emitting region or lower than solar metallicity.
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