The remarkable similarity of massive galaxy clusters from z~0 to z~1.9
Abstract
We present the results of a Chandra X-ray survey of the 8 most massive galaxy clusters at z > 1.2 in the South Pole Telescope 2500 deg2 survey. We combine this sample with previously-published Chandra observations of 49 massive X-ray-selected clusters at 0 < z < 0.1 and 90 SZ-selected clusters at 0.25 < z < 1.2 to constrain the evolution of the intracluster medium (ICM) over the past ~10 Gyr. We find that the bulk of the ICM has evolved self similarly over the full redshift range probed here, with the ICM density at r > 0.2R500 scaling like E(z) 2 . In the centers of clusters (r . 0.01R500), we find significant deviations from self similarity (ne ∝ E(z) 0.1±0.5 ), consistent with no redshift dependence. When we isolate clusters with over-dense cores (i.e., cool cores), we find that the average over-density profile has not evolved with redshift – that is, cool cores have not changed in size, density, or total mass over the past ~9–10 Gyr. We show that the evolving “cuspiness” of clusters in the Xray, reported by several previous studies, can be understood in the context of a cool core with fixed properties embedded inmore »
- Authors:
-
- Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States)
- Stanford Univ., Stanford, CA (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, Chicago, IL (United States)
- Univ. of Chicago, Chicago, IL (United States); Argonne National Lab. (ANL), Argonne, IL (United States)
- Univ. of Missouri, Columbia, MO (United States)
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Univ. de Montreal, Montreal, QC (Canada)
- Huntingdon Institute for X-ray Astronomy, Huntingdon, PA (United States)
- Princeton Univ., Princeton, NJ (United States)
- Univ. of Chicago, Chicago, IL (United States)
- Publication Date:
- Research Org.:
- SLAC National Accelerator Lab., Menlo Park, CA (United States); Argonne National Lab. (ANL), Argonne, IL (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF); National Aeronautics and Space Administration (NASA); USDOE Office of Science (SC), Basic Energy Sciences (BES); Gordon and Betty Moore Foundation
- Contributing Org.:
- SPT
- OSTI Identifier:
- 1369250
- Alternate Identifier(s):
- OSTI ID: 1352199; OSTI ID: 1373896
- Report Number(s):
- FERMILAB-PUB-17-072-AE; arXiv:1702.05094
Journal ID: ISSN 1538-4357
- Grant/Contract Number:
- AC02-76SF00515; AC02-07CH11359; AC02-06CH11357
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 843; Journal Issue: 1; Journal ID: ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; galaxies: clusters: general; galaxies: clusters: intracluster medium; galaxies: high-redshift; X-rays: galaxies: clusters
Citation Formats
McDonald, M., Allen, S. W., Bayliss, M., Benson, B. A., Bleem, L. E., Brodwin, M., Bulbul, E., Carlstrom, J. E., Forman, W. R., Hlavacek-Larrondo, J., Garmire, G. P., Gaspari, M., Gladders, M. D., Mantz, A. B., and Murray, S. S. The remarkable similarity of massive galaxy clusters from z~0 to z~1.9. United States: N. p., 2017.
Web. doi:10.3847/1538-4357/aa7740.
McDonald, M., Allen, S. W., Bayliss, M., Benson, B. A., Bleem, L. E., Brodwin, M., Bulbul, E., Carlstrom, J. E., Forman, W. R., Hlavacek-Larrondo, J., Garmire, G. P., Gaspari, M., Gladders, M. D., Mantz, A. B., & Murray, S. S. The remarkable similarity of massive galaxy clusters from z~0 to z~1.9. United States. https://doi.org/10.3847/1538-4357/aa7740
McDonald, M., Allen, S. W., Bayliss, M., Benson, B. A., Bleem, L. E., Brodwin, M., Bulbul, E., Carlstrom, J. E., Forman, W. R., Hlavacek-Larrondo, J., Garmire, G. P., Gaspari, M., Gladders, M. D., Mantz, A. B., and Murray, S. S. Wed .
"The remarkable similarity of massive galaxy clusters from z~0 to z~1.9". United States. https://doi.org/10.3847/1538-4357/aa7740. https://www.osti.gov/servlets/purl/1369250.
@article{osti_1369250,
title = {The remarkable similarity of massive galaxy clusters from z~0 to z~1.9},
author = {McDonald, M. and Allen, S. W. and Bayliss, M. and Benson, B. A. and Bleem, L. E. and Brodwin, M. and Bulbul, E. and Carlstrom, J. E. and Forman, W. R. and Hlavacek-Larrondo, J. and Garmire, G. P. and Gaspari, M. and Gladders, M. D. and Mantz, A. B. and Murray, S. S.},
abstractNote = {We present the results of a Chandra X-ray survey of the 8 most massive galaxy clusters at z > 1.2 in the South Pole Telescope 2500 deg2 survey. We combine this sample with previously-published Chandra observations of 49 massive X-ray-selected clusters at 0 < z < 0.1 and 90 SZ-selected clusters at 0.25 < z < 1.2 to constrain the evolution of the intracluster medium (ICM) over the past ~10 Gyr. We find that the bulk of the ICM has evolved self similarly over the full redshift range probed here, with the ICM density at r > 0.2R500 scaling like E(z) 2 . In the centers of clusters (r . 0.01R500), we find significant deviations from self similarity (ne ∝ E(z) 0.1±0.5 ), consistent with no redshift dependence. When we isolate clusters with over-dense cores (i.e., cool cores), we find that the average over-density profile has not evolved with redshift – that is, cool cores have not changed in size, density, or total mass over the past ~9–10 Gyr. We show that the evolving “cuspiness” of clusters in the Xray, reported by several previous studies, can be understood in the context of a cool core with fixed properties embedded in a self similarly-evolving cluster. We find no measurable evolution in the X-ray morphology of massive clusters, seemingly in tension with the rapidly-rising (with redshift) rate of major mergers predicted by cosmological simulations. We show that these two results can be brought into agreement if we assume that the relaxation time after a merger is proportional to the crossing time, since the latter is proportional to H(z) -1.},
doi = {10.3847/1538-4357/aa7740},
journal = {The Astrophysical Journal (Online)},
number = 1,
volume = 843,
place = {United States},
year = {Wed Jun 28 00:00:00 EDT 2017},
month = {Wed Jun 28 00:00:00 EDT 2017}
}
Web of Science
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X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field
journal, November 2019
- Ota, Naomi; Mitsuishi, Ikuyuki; Babazaki, Yasunori
- Publications of the Astronomical Society of Japan
JVLA 1.5 GHz Continuum Observation of CLASH Clusters. I. Radio Properties of the BCGs
journal, January 2018
- Yu, Heng; Tozzi, Paolo; van Weeren, Reinout
- The Astrophysical Journal, Vol. 853, Issue 2
Revisiting the Cooling Flow Problem in Galaxies, Groups, and Clusters of Galaxies
journal, May 2018
- McDonald, M.; Gaspari, M.; McNamara, B. R.
- The Astrophysical Journal, Vol. 858, Issue 1
X-Ray Properties of AGN in Brightest Cluster Galaxies. I. A Systematic Study of the Chandra Archive in the 0.2 < z < 0.3 and 0.55 < z < 0.75 Redshift Range
journal, May 2018
- Yang, Lilan; Tozzi, Paolo; Yu, Heng
- The Astrophysical Journal, Vol. 859, Issue 1
A Galaxy-scale Fountain of Cold Molecular Gas Pumped by a Black Hole
journal, September 2018
- Tremblay, G. R.; Combes, F.; Oonk, J. B. R.
- The Astrophysical Journal, Vol. 865, Issue 1
Spectroscopic Confirmation of Five Galaxy Clusters at z > 1.25 in the 2500 deg 2 SPT-SZ Survey
journal, December 2018
- Khullar, G.; Bleem, L. E.; Bayliss, M. B.
- The Astrophysical Journal, Vol. 870, Issue 1
A Detailed Study of the Most Relaxed SPT-selected Galaxy Clusters: Properties of the Cool Core and Central Galaxy
journal, January 2019
- McDonald, M.; Allen, S. W.; Hlavacek-Larrondo, J.
- The Astrophysical Journal, Vol. 870, Issue 2
The Impact of Radio AGN Bubble Composition on the Dynamics and Thermal Balance of the Intracluster Medium
journal, January 2019
- Yang, H. -Y. Karen; Gaspari, Massimo; Marlow, Carl
- The Astrophysical Journal, Vol. 871, Issue 1
Cluster Cosmology Constraints from the 2500 deg 2 SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
journal, June 2019
- Bocquet, S.; Dietrich, J. P.; Schrabback, T.
- The Astrophysical Journal, Vol. 878, Issue 1
Expanding the Sample of Radio Minihalos in Galaxy Clusters
journal, July 2019
- Giacintucci, Simona; Markevitch, Maxim; Cassano, Rossella
- The Astrophysical Journal, Vol. 880, Issue 2
On the Assembly Bias of Cool Core Clusters Traced by H α Nebulae
journal, September 2019
- Medezinski, Elinor; McDonald, Michael; More, Surhud
- The Astrophysical Journal, Vol. 882, Issue 2
The X-Ray Halo Scaling Relations of Supermassive Black Holes
journal, October 2019
- Gaspari, M.; Eckert, D.; Ettori, S.
- The Astrophysical Journal, Vol. 884, Issue 2
Probing the Origin of Diffuse Radio Emission in the Cool Core of the Phoenix Galaxy Cluster
journal, January 2020
- Raja, Ramij; Rahaman, Majidul; Datta, Abhirup
- The Astrophysical Journal, Vol. 889, Issue 2
Discovery of a Powerful >10 61 erg AGN Outburst in the Distant Galaxy Cluster SPT-CLJ0528-5300
journal, December 2019
- Calzadilla, Michael S.; McDonald, Michael; Bayliss, Matthew
- The Astrophysical Journal, Vol. 887, Issue 1
Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction
text, January 2018
- Barnes, David J.; Kannan, Rahul; Vogelsberger, Mark
- arXiv
Cluster Cosmology Constraints from the 2500 deg$^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
text, January 2018
- Bocquet, S.; Dietrich, J. P.; Schrabback, T.
- arXiv
The Three Hundred Project: The evolution of galaxy cluster density profiles
text, January 2018
- Mostoghiu, Robert; Knebe, Alexander; Cui, Weiguang
- arXiv
Constraining Gas Motions in the Intra-Cluster Medium
text, January 2019
- Simionescu, A.; ZuHone, J.; Zhuravleva, I.
- arXiv
Expanding the sample of radio minihalos in galaxy clusters
text, January 2019
- Giacintucci, Simona; Markevitch, Maxim; Cassano, Rossella
- arXiv
Probing the origin of diffuse radio emission in the cool-core of the Phoenix galaxy cluster
text, January 2019
- Raja, Ramij; Rahaman, Majidul; Datta, Abhirup
- arXiv