Physical conditions of the gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44

Huynh, M. T.; Norris, R. P.; Coppin, K. E. K.; Emonts, B. H. C.; Ivison, R. J.; Seymour, N.; Smail, I.; Smolčić, Vernesa; Swinbank, A. M.; Brandt, W. N.; Chapman, S. C.; Dannerbauer, H.; Breuck, C. De; Greve, T. R.; Hodge, J. A.; Karim, A.; Knudsen, K. K.; Menten, K. M.; van der Werf, P. P.; Walter, F.; Weiss, A.

doi:10.1093/mnrasl/slt014

prikaz prve stranice dokumenta Physical conditions of the gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44

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Physical conditions of the gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44

Monthly Notices of the Royal Astronomical Society, 431 (2013), 1; L88-L92. https://doi.org/10.1093/mnrasl/slt014

Huynh, M. T.; Norris, R. P.; Coppin, K. E. K.; Emonts, B. H. C.; Ivison, R. J.; Seymour, N.; Smail, I.; Smolčić, Vernesa; Swinbank, A. M.; Brandt, W. N.; Chapman, S. C.; Dannerbauer, H.; Breuck, C. De; Greve, T. R.; Hodge, J. A.; Karim, A.; Knudsen, K. K.; Menten, K. M.; van der Werf, P. P.; Walter, F.; Weiss, A. Više autora...

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APA 6th Edition

Huynh, M. T., Norris, R. P., Coppin, K. E. K., Emonts, B. H. C., Ivison, R. J., Seymour, N. ... Weiss, A. (2013). Physical conditions of the gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44. Monthly Notices of the Royal Astronomical Society, 431. (1), L88-L92. doi: 10.1093/mnrasl/slt014

MLA 8th Edition

Huynh, M. T., et al. "Physical conditions of the gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44." Monthly Notices of the Royal Astronomical Society, vol. 431, br. 1, 2013, str. L88-L92. https://doi.org/10.1093/mnrasl/slt014

Chicago 17th Edition

Huynh, M. T., R. P. Norris, K. E. K. Coppin, B. H. C. Emonts, R. J. Ivison, N. Seymour, I. Smail, et al. "Physical conditions of the gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44." Monthly Notices of the Royal Astronomical Society 431, br. 1 (2013): L88-L92. https://doi.org/10.1093/mnrasl/slt014

Harvard

Huynh, M. T., et al. (2013) 'Physical conditions of the gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44', Monthly Notices of the Royal Astronomical Society, 431(1), str. L88-L92. doi: 10.1093/mnrasl/slt014

Vancouver

Huynh MT, Norris RP, Coppin KEK, Emonts BHC, Ivison RJ, Seymour N, i sur.. Physical conditions of the gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44. Monthly Notices of the Royal Astronomical Society [Internet]. 2013. [pristupljeno 23.04.2024.];431(1):L88-L92. doi: 10.1093/mnrasl/slt014

IEEE

M. T. Huynh, et al., "Physical conditions of the gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44", Monthly Notices of the Royal Astronomical Society, vol. 431, br. 1, str. L88-L92, 2013. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:524602. [Citirano: 23.04.2024.]

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Naslov (engleski)	Physical conditions of the gas in an ALMA [C II]-identified submillimetre galaxy at z = 4.44
Autor	M. T. Huynh
Autor	R. P. Norris
Autor	K. E. K. Coppin
Autor	B. H. C. Emonts
Autor	R. J. Ivison
Autor	N. Seymour
Autor	I. Smail
Autor	Vernesa Smolčić
Autor	A. M. Swinbank
Autor	W. N. Brandt
Autor	S. C. Chapman
Autor	H. Dannerbauer
Autor	C. De Breuck
Autor	T. R. Greve
Autor	J. A. Hodge
Autor	A. Karim
Autor	K. K. Knudsen
Autor	K. M. Menten
Autor	P. P. van der Werf
Autor	F. Walter
Autor	A. Weiss
Autorova ustanova	Sveučilište u Zagrebu Prirodoslovno-matematički fakultet (Fizički odsjek)
Znanstveno / umjetničko područje, polje i grana	PRIRODNE ZNANOSTI Fizika
Sažetak (engleski)	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 M_gas < 1.7 x 10^{10} M_⊙. 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 G0 ≳ 10^3, as seen in Galactic star-forming regions or local ultraluminous infrared galaxies (ULIRGs). The observed L_{[C II]}/L_FIR = 2.3 x 10^{-3} is high compared to local ULIRGs and, combined with L_{[C II]}/L_CO ≳ 2700, it is consistent with ALESS65.1 either having an extended (several kpc) [C II] emitting region or lower than solar metallicity.
Ključne riječi (engleski)
Jezik	engleski
Vrsta publikacije	Znanstveni rad - Izvorni znanstveni rad
Status objave	Objavljen
Vrsta recenzije	Recenziran - međunarodna recenzija
Verzija publikacije	Objavljena verzija rada (izdavačev PDF)
Naslov časopisa	Monthly Notices of the Royal Astronomical Society
Brojčani podaci	vol. 431, br. 1, str. L88-L92
p-ISSN	0035-8711
e-ISSN	1365-2966
DOI	https://doi.org/10.1093/mnrasl/slt014
URN:NBN	urn:nbn:hr:217:524602
Datum objave publikacije	2013
URL dokumenta	https://academic.oup.com/mnrasl/article/431/1/L88/1409514
Vrsta resursa	Tekst
Prava pristupa	Otvoreni pristup
Uvjeti korištenja
Javna napomena	© 2013 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. Accepted 2013 January 30. Received 2013 January 29; in original form 2012 December 10. First published online March 7, 2013.
Datum i vrijeme pohrane	2019-11-25 20:04:58