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

Author(s):: Turner, M.L.; Schaye, J. (0000-0002-0668-5560); Crain, R.A.; Rudie, G.; Steidel, C.C.; Strom, A.; Theuns, T.

Published: 2017
Publication type: Article / Letter to editor

Date issued: 2017
Language: English
Is part of: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (ISSN 0035-8711) (2017), Vol. 471, p. 690-705
hdl: 1887/58809
doi: 10.1093/mnras/stx1616
URL: https://arxiv.org/abs/1703.00086