Resolving CO (2-1) in z ~ 1.6 Gas-rich Cluster Galaxies with ALMA: Rotating Molecular Gas Disks with Possible Signatures of Gas Stripping (2019)
Attributed to:
Ascertaining the mechanism behind satellite quenching in high-redshift galaxy clusters
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aaf1c6
Publication URI: http://dx.doi.org/10.3847/1538-4357/aaf1c6
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2