The SAMI Galaxy Survey: Mass as the Driver of the Kinematic Morphology-Density Relation in Clusters (2017)
Attributed to:
Astrophysics and Planetary Science at Oxford 2013-16
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aa7a11
Publication URI: http://dx.doi.org/10.3847/1538-4357/aa7a11
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 1