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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

ABSTRACT 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 ( ) clusters of galaxies selected by their Sunyaev-Zel'dovich...

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Published in:The Astrophysical journal 2015-05, Vol.805 (1), p.1-13
Main Authors: Hlavacek-Larrondo, J., McDonald, M., Benson, B. A., Forman, W. R., Allen, S. W., Bleem, L. E., Ashby, M. L. N., Bocquet, S., Brodwin, M., Dietrich, J. P., Jones, C., Liu, J., Reichardt, C. L., Saliwanchik, B. R., Saro, A., Schrabback, T., Song, J., Stalder, B., Vikhlinin, A., Zenteno, A.
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Language:English
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Summary:ABSTRACT 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 ( ) clusters of galaxies selected by their Sunyaev-Zel'dovich signature in the South Pole Telescope data. Based on Chandra X-ray images, we find a total of six clusters having symmetric pairs of surface brightness depressions consistent with the picture of radio jets inflating X-ray cavities in the intracluster medium (ICM). The majority of these detections are of relatively low significance and require deeper follow-up data in order to be confirmed. Further, this search will miss small (
ISSN:0004-637X
1538-4357
1538-4357
DOI:10.1088/0004-637X/805/1/35