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

Sebastian Lopez (), Nicolas Tejos, Cédric Ledoux, L. Felipe Barrientos, Keren Sharon, Jane R. Rigby, Michael D. Gladders, Matthew B. Bayliss and Ismael Pessa
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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
Matthew B. Bayliss: Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology
Ismael Pessa: Instituto de Astrofísica, Pontificia Universidad Católica de Chile

Nature, 2018, vol. 554, issue 7693, 493-496

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.

Date: 2018
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DOI: 10.1038/nature25436

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