Rotation in [C ii]-emitting gas in two galaxies at a redshift of 6.8

Renske Smit (), Rychard J. Bouwens, Stefano Carniani, Pascal A. Oesch, Ivo Labbé, Garth D. Illingworth, Paul van der Werf, Larry D. Bradley, Valentino Gonzalez, Jacqueline A. Hodge, Benne W. Holwerda, Roberto Maiolino and Wei Zheng
Additional contact information
Renske Smit: Cavendish Laboratory, University of Cambridge
Rychard J. Bouwens: Leiden Observatory, Leiden University
Stefano Carniani: Cavendish Laboratory, University of Cambridge
Pascal A. Oesch: Observatoire de Genève, Université de Genève
Ivo Labbé: Leiden Observatory, Leiden University
Garth D. Illingworth: UCO/Lick Observatory, University of California, Santa Cruz
Paul van der Werf: Leiden Observatory, Leiden University
Larry D. Bradley: Space Telescope Science Institute
Valentino Gonzalez: Universidad de Chile
Jacqueline A. Hodge: Leiden Observatory, Leiden University
Benne W. Holwerda: University of Louisville
Roberto Maiolino: Cavendish Laboratory, University of Cambridge
Wei Zheng: The Johns Hopkins University

Nature, 2018, vol. 553, issue 7687, 178-181

Abstract: The emission of singly ionized carbon is used to identify two galaxies with redshifts of nearly 7—corresponding to the Universe’s first billion years—and with velocity structures suggestive of rotation.

Date: 2018
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DOI: 10.1038/nature24631

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