Mapping the dynamics of a giant Ly a halo at z = 4.1 with MUSE: the energetics of a large-scale AGN-driven outflow around a massive, high-redshift galaxy (2015)
Attributed to:
The Spatially Resolved Kinematics, Star-Formation and Chemical Adundances of High-Redshift Galaxies
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stv366
Publication URI: http://dx.doi.org/10.1093/mnras/stv366
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 2