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The nature of the variable millimetre–selected AGN in the brightest cluster galaxy of Abell 851

Cheale, RA; Geach, JE; Edge, AC; Perrott, YC; Cantwell, T

The nature of the variable millimetre–selected AGN in the brightest cluster galaxy of Abell 851 Thumbnail


Authors

RA Cheale

JE Geach

YC Perrott

T Cantwell



Abstract

We present the detection of a bright 3 mm continuum source in the brightest cluster galaxy (BCG) in Abell 0851 (z = 0.411) with the NOrthern Extended Millimeter Array (NOEMA). When this detection is compared to other multifrequency observations across 21cm– 100μm, including new Arcminute Microkelvin Imager 15 GHz observations, we find evidence for a relatively flat, variable core source associated with the BCG. The radio power and amplitude of variability observed in this galaxy is consistent with the cores in lower redshift BCGs in X-ray–selected clusters, and the flat mm–cm spectrum is suggestive of the BCG being a low-luminosity active galactic nucleus archetype. The discovery of this system could provide a basis for a long-term study of the role of low-luminosity radio mode ‘regulatory’ feedback in massive clusters.

Citation

Cheale, R., Geach, J., Edge, A., Perrott, Y., & Cantwell, T. (2018). The nature of the variable millimetre–selected AGN in the brightest cluster galaxy of Abell 851. Monthly Notices of the Royal Astronomical Society: Letters, 481(1), L54-L58. https://doi.org/10.1093/mnrasl/sly161

Journal Article Type Article
Acceptance Date Aug 25, 2018
Online Publication Date Aug 31, 2018
Publication Date Aug 31, 2018
Deposit Date Sep 24, 2018
Publicly Available Date Oct 10, 2018
Journal Monthly Notices of the Royal Astronomical Society: Letters
Electronic ISSN 1745-3933
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 481
Issue 1
Pages L54-L58
DOI https://doi.org/10.1093/mnrasl/sly161
Related Public URLs https://arxiv.org/pdf/1809.01700.pdf

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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2018 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.





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