$The absence of [C ii ] 158 $\mu$m emission in spectroscopically confirmed galaxies at z > 8$

The absence of [C ii ] 158 $\mu$m emission in spectroscopically confirmed galaxies at z > 8

The scatter in the relationship between the strength of [C ii] 158 $\mu$m emission and the star formation rate at high redshift has been the source of much recent interest. Although the relationship is well established locally, several intensely star-forming galaxies have been found whose [C ii] 158...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2019-07, Vol.487 (1), p.L81-L85
Hauptverfasser:	Laporte, N, Katz, H, Ellis, R S, Lagache, G, Bauer, F E, Boone, F, Inoue, A K, Hashimoto, T, Matsuo, H, Mawatari, K, Tamura, Y
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Physics
Online-Zugang:	Volltext
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