The spatial correlation of bent-tail galaxies and galaxy clusters

12Citations
Citations of this article
11Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

We have completed a deep radio continuum survey covering 86 deg2 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 eight 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.

Cite

CITATION STYLE

APA

O’Brien, A. N., Norris, R. P., Tothill, N. F. H., & Filipović, M. D. (2018). The spatial correlation of bent-tail galaxies and galaxy clusters. Monthly Notices of the Royal Astronomical Society, 481(4), 5247–5262. https://doi.org/10.1093/MNRAS/STY2642

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free