The SAMI Galaxy Survey: Mass as the Driver of the Kinematic Morphology-Density Relation in Clusters (2024)
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/10.25916/sut.26244764
Type: Other