The SAMI Galaxy Survey: mass as the driver of the kinematic morphology - density relation in clusters (2017)

First Author: Brough S
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/10.48550/arxiv.1704.01169

Publication URI: https://arxiv.org/abs/1704.01169

Type: Other