arXiv Analytics

Sign in

arXiv:1809.10346 [astro-ph.GA]AbstractReferencesReviewsResources

The Spatial Correlation of Bent-Tail Galaxies and Galaxy Clusters

Andrew N. O'Brien, Ray P. Norris, Nick F. H. Tothill, Miroslav D. Filipović

Published 2018-09-27Version 1

We have completed a deep radio continuum survey covering 86 square degrees of the Spitzer-South Pole Telescope deep field to test whether bent-tail galaxies are associated with galaxy clusters. We present a new catalogue of 22 bent-tail galaxies and a further 24 candidate bent-tail galaxies. Surprisingly, of the 8 bent-tail galaxies with photometric redshifts, only two are associated with known clusters. While the absence of bent-tail sources in known clusters may be explained by effects such as sensitivity, the absence of known clusters associated with most bent-tail galaxies casts doubt upon current models of bent-tail galaxies.

Related articles: Most relevant | Search more
arXiv:1603.03524 [astro-ph.GA] (Published 2016-03-11)
Baryon content and dynamic state of galaxy clusters: XMM-Newton observations of A1095 and A1926
arXiv:1806.08822 [astro-ph.GA] (Published 2018-06-22)
Cooling+Heating Flows in Galaxy clusters: Turbulent heating, spectral modelling, and cold mass budget
arXiv:1407.5729 [astro-ph.GA] (Published 2014-07-22)
Metal distribution in the ICM - a comprehensive numerical study of twelve galaxy clusters