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Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 1(471), p. 690-705, 2017

DOI: 10.1093/mnras/stx1616

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A comparison of observed and simulated absorption from H i, C iv, and Si iv around z ≈ 2 star-forming galaxies suggests redshift–space distortions are due to inflows

Journal article published in 2017 by Monica L. Turner ORCID, Joop Schaye ORCID, Robert A. Crain ORCID, Gwen Rudie, Charles C. Steidel ORCID, Allison Strom, Tom Theuns
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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