X-RAY CAVITIES IN A SAMPLE OF 83 SPT-SELECTED CLUSTERS OF GALAXIES: TRACING THE EVOLUTION OF AGN FEEDBACK IN CLUSTERS OF GALAXIES OUT TO z = 1.2

X-ray cavities are key tracers of mechanical (or radio mode) heating arising from the active galactic nuclei (AGNs) in brightest cluster galaxies (BCGs). We report on a survey for X-ray cavities in 83 massive, high-redshift (0.4 < z < 1.2) clusters of galaxies selected by their Sunyaev-Zel...

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Bibliographic Details
Main Authors: Hlavacek-Larrondo, J. (Author), Benson, B. A. (Author), Forman, W. R. (Author), Allen, S. W. (Author), Bleem, L. E. (Author), Ashby, M. L. N. (Author), Bocquet, S. (Author), Brodwin, M. (Author), Dietrich, J. P. (Author), Jones, C. (Author), Liu, J. (Author), Reichardt, C. L. (Author), Saliwanchik, B. R. (Author), Saro, A. (Author), Schrabback, T. (Author), Song, J. (Author), Stalder, B. (Author), Vikhlinin, A. (Author), Zenteno, A. (Author), McDonald, Michael A. (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-09-03T18:41:56Z.
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