[C ii] 158-μm emission from the host galaxies of damped Lyman-alpha systems

Gas surrounding high-redshift galaxies has been studied through observations of absorption line systems toward background quasars for decades. However, it has proven difficult to identify and characterize the galaxies associated with these absorbers due to the intrinsic faintness of the galaxies com...

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Veröffentlicht in:	Science (American Association for the Advancement of Science) 2017-03, Vol.355 (6331), p.1285-1288
Hauptverfasser:	Neeleman, Marcel, Kanekar, Nissim, Prochaska, J. Xavier, Rafelski, Marc, Carilli, Chris L., Wolfe, Arthur M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Absorption Arrays Emission Enrichment Galaxies Hydrogen Quasars Star formation
Online-Zugang:	Volltext
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