[C ii] emission in z ∼ 6 strongly lensed, star-forming galaxies

[C ii] emission in z ∼ 6 strongly lensed, star-forming galaxies

The far-infrared fine-structure line [C II] at 1900.5 GHz is known to be one of the brightest cooling lines in local galaxies, and therefore it has been suggested to be an efficient tracer for star formation in very high redshift galaxies. However, recent results for galaxies at z > 6 have yielde...

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Bibliographic Details
Main Authors:	Knudsen, Kirsten K., Richard, Johan, Kneib, Jean-Paul, Jauzac, Mathilde, Clément, Benjamin, Drouart, Guillaume, Egami, Eiichi, Lindroos, Lukas
Other Authors:	Univ Arizona, Steward Observ
Language:	en
Published:	OXFORD UNIV PRESS 2016
Subjects:	galaxies: evolution galaxies: formation galaxies: high-redshift galaxies: ISM submillimetre: galaxies
Online Access:	http://hdl.handle.net/10150/621730 http://arizona.openrepository.com/arizona/handle/10150/621730

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