posted on 2024-08-06, 10:36authored byPaola Oliva Altamirano, Sarah Brough, Kim-Vy Tran, Jimmy, Christopher Miller, Malcom N. Bremer, Steven Phillipps, Rob Sharp, Matthew Colless, Maritza A. Lara-López, Ángel R. López-Sánchez, Kevin Pimbblet, Prajwal R. Kafle, Warrick CouchWarrick Couch
We present a pilot analysis of the influence of galaxy stellar mass and cluster environment on the probability of slow rotation in 22 central galaxies at mean redshift z=0.07. This includes new integral-field observations of 5 central galaxies selected from the Sloan Digital Sky Survey, observed with the SPIRAL integral-field spectrograph on the Anglo-Australian Telescope. The composite sample presented here spans a wide range of stellar masses, 10.9