Dust-obscured star formation in the outskirts of XMMU J2235.3-2557, a massive galaxy cluster at z = 1.4? (2013)
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/stt811
Publication URI: http://dx.doi.org/10.1093/mnras/stt811
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 2