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A STUDY of CENTRAL GALAXY ROTATION with STELLAR MASS and ENVIRONMENT

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posted on 2024-08-06, 10:36 authored by Paola 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

Funding

Investigating Rosetta Stones of galaxy formation

Australian Research Council

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Monster galaxies: Extreme limits on galaxy formation

Australian Research Council

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ISSN

0004-6256

Journal title

Astronomical Journal

Volume

153

Issue

2

Pagination

1 p

Publisher

IOP Publishing

Copyright statement

Copyright © 2017. The American Astronomical Society. All rights reserved. The published version is reproduced here in accordance with the copyright policy of the publisher and can be also be located at https://doi.org/10.3847/1538-3881/153/2/89.

Language

eng

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