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

Author

Listed:
  • Renske Smit

    (Cavendish Laboratory, University of Cambridge
    Kavli Institute for Cosmology, University of Cambridge)

  • Rychard J. Bouwens

    (Leiden Observatory, Leiden University)

  • Stefano Carniani

    (Cavendish Laboratory, University of Cambridge
    Kavli Institute for Cosmology, 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
    Centro de Astrofisica y Tecnologias Afines (CATA))

  • Jacqueline A. Hodge

    (Leiden Observatory, Leiden University)

  • Benne W. Holwerda

    (University of Louisville)

  • Roberto Maiolino

    (Cavendish Laboratory, University of Cambridge
    Kavli Institute for Cosmology, University of Cambridge)

  • Wei Zheng

    (The Johns Hopkins University)

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.

Suggested Citation

  • 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. Ho, 2018. "Rotation in [C ii]-emitting gas in two galaxies at a redshift of 6.8," Nature, Nature, vol. 553(7687), pages 178-181, January.
    • Handle: RePEc:nat:nature:v:553:y:2018:i:7687:d:10.1038_nature24631
    DOI: 10.1038/nature24631
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