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A clumpy and anisotropic galaxy halo at redshift 1 from gravitational-arc tomography

Author

Listed:
  • Sebastian Lopez

    (Universidad de Chile)

  • Nicolas Tejos

    (Instituto de Física, Pontificia Universidad Católica de Valparaíso)

  • Cédric Ledoux

    (European Southern Observatory)

  • L. Felipe Barrientos

    (Instituto de Astrofísica, Pontificia Universidad Católica de Chile)

  • Keren Sharon

    (University of Michigan)

  • Jane R. Rigby

    (Observational Cosmology Laboratory, NASA Goddard Space Flight Center)

  • Michael D. Gladders

    (University of Chicago
    Kavli Institute for Cosmological Physics, University of Chicago)

  • Matthew B. Bayliss

    (Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology)

  • Ismael Pessa

    (Instituto de Astrofísica, Pontificia Universidad Católica de Chile)

Abstract

The halo of gas around a galaxy at redshift 1 is clumpy and anisotropic, with little variation in gas velocity, suggesting that it consists of entrained recycled material.

Suggested Citation

  • Sebastian Lopez & Nicolas Tejos & Cédric Ledoux & L. Felipe Barrientos & Keren Sharon & Jane R. Rigby & Michael D. Gladders & Matthew B. Bayliss & Ismael Pessa, 2018. "A clumpy and anisotropic galaxy halo at redshift 1 from gravitational-arc tomography," Nature, Nature, vol. 554(7693), pages 493-496, February.
  • Handle: RePEc:nat:nature:v:554:y:2018:i:7693:d:10.1038_nature25436
    DOI: 10.1038/nature25436
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