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

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.

doi:10.1088/0004-637X/805/1/35

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

Journal Article · Mon May 18 00:00:00 EDT 2015 · The Astrophysical Journal (Online)

DOI:https://doi.org/10.1088/0004-637X/805/1/35· OSTI ID:1336376

^[1]; ^[2]; Benson, B. A. ^[3]; Forman, W. R. ^[4]; Allen, S. W. ^[5]; Bleem, L. E. ^[6]; Ashby, M. L. N. ^[4]; ^[7]; ^[8]; Dietrich, J. P. ^[7]; Jones, C. ^[4]; Liu, J. ^[7]; Reichardt, C. L. ^[9]; Saliwanchik, B. R. ^[10]; Saro, A. ^[11]; Schrabback, T. ^[12]; Song, J. ^[13]; Stalder, B. ^[14]; Vikhlinin, A. ^[4]; Zenteno, A. ^[15]

Univ. of Montreal, Quebec (Canada). Dept. of Physics; Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology and Dept. of Physics
Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States). Kavli Inst. for Astrophysics and Space Research
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics and Dept. of Astronomy and Astrophysics; Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology and Dept. of Physics; SLAC National Accelerator Lab., Menlo Park, CA (United States)
Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP) and Dept. of Physics; Argonne National Lab. (ANL), Argonne, IL (United States)
Ludwig Maximilian Univ., Munich (Germany); Excellence Cluster Univ., Garching (Germany)
Univ. of Missouri, Kansas City, MO (United States). Dept. of Physics and Astronomy
Univ. of California, Berkeley, CA (United States). Dept. of Physics; Univ. of Melbourne (Australia). School of Physics
Case Western Reserve Univ., Cleveland, OH (United States). Cetner for Education and Research in Cosmology and Astrophysics
Ludwig Maximilian Univ., Munich (Germany). Dept. of Physics
Argelander Institute for Astronomy, Bonn (Germany)
Univ. of Michigan, Ann Arbor, MI (United States). Dept. of Physics; Korea Astronomy and Space Science Inst., Daejeon (Korea)
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States); Univ. of Hawaii, Honolulu, HI (United States). Inst. for Astronomy
Ludwig Maximilian Univ., Munich (Germany); Cerro Tololo Inter-American Observatory (CTIO), La Serena (Chile)

X-ray cavities are key tracers of mechanical (or radio mode) heating arising from the active galactic nuclei (AGNs) in brightest cluster galaxies (BCGs). Here, we report on a survey for X-ray cavities in 83 massive, high-redshift ($$0.4\lt z\lt 1.2$$) 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). Furthermore, 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 (<10 kpc) X-ray cavities that are unresolved by Chandra at high ($$z\gtrsim 0.5$$) redshift. Despite these limitations, our results suggest that the power generated by AGN feedback in BCGs has remained unchanged for over half of the age of the universe ($$\gt 7$$ Gyr at $$z\sim 0.8$$). On average, the detected X-ray cavities have powers of $$(0.8-5)\times {{10}^{45}}\ {\rm erg}\ {{{\rm s}}^{-1}}$$, enthalpies of $$(3-6)\times {{10}^{59}}\ {\rm erg}$$, and radii of ~17 kpc. Integrating over 7 Gyr, we find that the supermassive black holes in BCGs may have accreted 108 to several $${{10}^{9}}\;{{M}_{\odot }}$$ of material to power these outflows. This level of accretion indicates that significant supermassive black hole growth may occur not only at early times, in the quasar era, but at late times as well. We also find that X-ray cavities at high redshift may inject an excess heat of 0.1–1.0 keV per particle into the hot ICM above and beyond the energy needed to offset cooling. Though our result needs to be confirmed, we note that the magnitude of excess heating is similar to the energy needed to preheat clusters, break self-similarity, and explain the excess entropy in hot atmospheres.

View Accepted Manuscript (DOE)

Research Organization:: SLAC National Accelerator Lab., Menlo Park, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: AC02-06CH11357; AC02-76SF00515

OSTI ID:: 1336376

Alternate ID(s):: OSTI ID: 1326609
OSTI ID: 1339659
OSTI ID: 22883194

Report Number(s):: SLAC-PUB--16762

Journal Information:: The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 1 Vol. 805; ISSN 1538-4357

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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Radio and X-Ray Detectability of Buoyant Radio Plasma Bubbles in Clusters of Galaxies Ensslin, Torsten A.; Heinz, Sebastian arXiv https://doi.org/10.48550/arxiv.astro-ph/0202101	text	January 2002
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The Integrated Sunyaev-Zeldovich Effect as the Superior Method for Measuring the Mass of Clusters of Galaxies Motl, Patrick M.; Hallman, Eric J.; Burns, Jack O. arXiv https://doi.org/10.48550/arxiv.astro-ph/0502226	text	January 2005
Chandra sample of nearby relaxed galaxy clusters: mass, gas fraction, and mass-temperature relation Vikhlinin, A.; Kravtsov, A.; Forman, W. arXiv https://doi.org/10.48550/arxiv.astro-ph/0507092	text	January 2005
A very deep Chandra observation of the Perseus cluster: shocks, ripples and conduction Fabian, A. C.; Sanders, J. S.; Taylor, G. B. arXiv https://doi.org/10.48550/arxiv.astro-ph/0510476	text	January 2005
Investigating AGN Heating in a Sample of Nearby Clusters Dunn, R. J. H.; Fabian, A. C. arXiv https://doi.org/10.48550/arxiv.astro-ph/0609537	text	January 2006
Analytical Models For Galactic Nuclei Zhao, HongSheng arXiv https://doi.org/10.48550/arxiv.astro-ph/9509122	text	January 1995
The Demography of Massive Dark Objects in Galaxy Centres Magorrian, John; Tremaine, Scott; Richstone, Douglas arXiv https://doi.org/10.48550/arxiv.astro-ph/9708072	text	January 1997
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