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

We examine the kinematic morphology of early-type galaxies (ETGs) in eight galaxy clusters in the Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey. The clusters cover a mass range of 14.2 : Accepted by ApJ 15 June 2017

Bibliographic Details
Main Authors:	Brough, Sarah, van de Sande, Jesse, Owers, Matt S., d'Eugenio, Francesco, Sharp, Rob, Cortese, Luca, Scott, Nicholas, Croom, Scott M., Bassett, Rob, Bekki, Kenji, Bland-Hawthorn, Joss, Bryant, Julia J., Davies, Roger, Drinkwater, Michael J., Driver, Simon P., Foster, Caroline, Goldstein, Gregory, Lopez-Sanchez, A. R., Medling, Anne M., Sweet, Sarah M., Taranu, Dan S., Tonini, Chiara, Yi, Sukyoung K., Goodwin, Michael, Lawrence, J. S., Richards, Samuel N.
Format:	Text
Language:	unknown
Published:	arXiv 2017
Subjects:	Astrophysics of Galaxies astro-ph.GA FOS Physical sciences sami
Online Access:	https://dx.doi.org/10.48550/arxiv.1704.01169 https://arxiv.org/abs/1704.01169

Description
Summary:	We examine the kinematic morphology of early-type galaxies (ETGs) in eight galaxy clusters in the Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey. The clusters cover a mass range of 14.2 : Accepted by ApJ 15 June 2017