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 (2017)
Attributed to:
Durham Astronomy Consolidated Grant 2017-2020
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stx1616
Publication URI: http://dx.doi.org/10.1093/mnras/stx1616
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 1