Evidence for AGN-regulated Cooling in Clusters at z ∼ 1.4: A Multiwavelength View of SPT-CL J0607-4448
We present a multiwavelength analysis of the galaxy cluster SPT-CL J0607-4448 (SPT0607), which is one of the most distant clusters discovered by the South Pole Telescope at z = 1.4010 ± 0.0028. The high-redshift cluster shows clear signs of being relaxed with well-regulated feedback from the active...
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ftdoajarticles:oai:doaj.org/article:43a3ed7fb69d400dbfbd03fa18d00080 2023-10-09T21:55:59+02:00 Evidence for AGN-regulated Cooling in Clusters at z ∼ 1.4: A Multiwavelength View of SPT-CL J0607-4448 Megan Masterson Michael McDonald Behzad Ansarinejad Matthew Bayliss Bradford A. Benson Lindsey E. Bleem Michael S. Calzadilla Alastair C. Edge Benjamin Floyd Keunho J. Kim Gourav Khullar Taweewat Somboonpanyakul 2023-01-01T00:00:00Z https://doi.org/10.3847/1538-4357/acae9e https://doaj.org/article/43a3ed7fb69d400dbfbd03fa18d00080 EN eng IOP Publishing https://doi.org/10.3847/1538-4357/acae9e https://doaj.org/toc/1538-4357 doi:10.3847/1538-4357/acae9e 1538-4357 https://doaj.org/article/43a3ed7fb69d400dbfbd03fa18d00080 The Astrophysical Journal, Vol 944, Iss 2, p 164 (2023) Brightest cluster galaxies Galaxy clusters Intracluster medium Radio galaxies High-redshift galaxy clusters Astrophysics QB460-466 article 2023 ftdoajarticles https://doi.org/10.3847/1538-4357/acae9e 2023-09-10T00:41:48Z We present a multiwavelength analysis of the galaxy cluster SPT-CL J0607-4448 (SPT0607), which is one of the most distant clusters discovered by the South Pole Telescope at z = 1.4010 ± 0.0028. The high-redshift cluster shows clear signs of being relaxed with well-regulated feedback from the active galactic nucleus (AGN) in the brightest cluster galaxy (BCG). Using Chandra X-ray data, we construct thermodynamic profiles and determine the properties of the intracluster medium. The cool-core nature of the cluster is supported by a centrally peaked density profile and low central entropy ( ${K}_{0}={18}_{-9}^{+11}$ keV cm ^2 ), which we estimate assuming an isothermal temperature profile due to the limited spectral information given the distance to the cluster. Using the density profile and gas cooling time inferred from the X-ray data, we find a mass-cooling rate ${\dot{M}}_{\mathrm{cool}}={100}_{-60}^{+90}\,{M}_{\odot }$ yr ^−1 . From optical spectroscopy and photometry around the [O ii ] emission line, we estimate that the BCG star formation rate is ${\mathrm{SFR}}_{[{\rm{O}}\,{\rm\small{II}}]}={1.7}_{-0.6}^{+1.0}\,{M}_{\odot }$ yr ^−1 , roughly two orders of magnitude lower than the predicted mass-cooling rate. In addition, using ATCA radio data at 2.1 GHz, we measure a radio jet power ${P}_{\mathrm{cav}}={3.2}_{-1.3}^{+2.1}\times {10}^{44}$ erg s ^−1 , which is consistent with the X-ray cooling luminosity ( ${L}_{\mathrm{cool}}={1.9}_{-0.5}^{+0.2}\times {10}^{44}$ erg s ^−1 within r _cool = 43 kpc). These findings suggest that SPT0607 is a relaxed, cool-core cluster with AGN-regulated cooling at an epoch shortly after cluster formation, implying that the balance between cooling and feedback can be reached quickly. We discuss the implications for these findings on the evolution of AGN feedback in galaxy clusters. Article in Journal/Newspaper South pole Directory of Open Access Journals: DOAJ Articles South Pole The Astrophysical Journal 944 2 164 |
institution |
Open Polar |
collection |
Directory of Open Access Journals: DOAJ Articles |
op_collection_id |
ftdoajarticles |
language |
English |
topic |
Brightest cluster galaxies Galaxy clusters Intracluster medium Radio galaxies High-redshift galaxy clusters Astrophysics QB460-466 |
spellingShingle |
Brightest cluster galaxies Galaxy clusters Intracluster medium Radio galaxies High-redshift galaxy clusters Astrophysics QB460-466 Megan Masterson Michael McDonald Behzad Ansarinejad Matthew Bayliss Bradford A. Benson Lindsey E. Bleem Michael S. Calzadilla Alastair C. Edge Benjamin Floyd Keunho J. Kim Gourav Khullar Taweewat Somboonpanyakul Evidence for AGN-regulated Cooling in Clusters at z ∼ 1.4: A Multiwavelength View of SPT-CL J0607-4448 |
topic_facet |
Brightest cluster galaxies Galaxy clusters Intracluster medium Radio galaxies High-redshift galaxy clusters Astrophysics QB460-466 |
description |
We present a multiwavelength analysis of the galaxy cluster SPT-CL J0607-4448 (SPT0607), which is one of the most distant clusters discovered by the South Pole Telescope at z = 1.4010 ± 0.0028. The high-redshift cluster shows clear signs of being relaxed with well-regulated feedback from the active galactic nucleus (AGN) in the brightest cluster galaxy (BCG). Using Chandra X-ray data, we construct thermodynamic profiles and determine the properties of the intracluster medium. The cool-core nature of the cluster is supported by a centrally peaked density profile and low central entropy ( ${K}_{0}={18}_{-9}^{+11}$ keV cm ^2 ), which we estimate assuming an isothermal temperature profile due to the limited spectral information given the distance to the cluster. Using the density profile and gas cooling time inferred from the X-ray data, we find a mass-cooling rate ${\dot{M}}_{\mathrm{cool}}={100}_{-60}^{+90}\,{M}_{\odot }$ yr ^−1 . From optical spectroscopy and photometry around the [O ii ] emission line, we estimate that the BCG star formation rate is ${\mathrm{SFR}}_{[{\rm{O}}\,{\rm\small{II}}]}={1.7}_{-0.6}^{+1.0}\,{M}_{\odot }$ yr ^−1 , roughly two orders of magnitude lower than the predicted mass-cooling rate. In addition, using ATCA radio data at 2.1 GHz, we measure a radio jet power ${P}_{\mathrm{cav}}={3.2}_{-1.3}^{+2.1}\times {10}^{44}$ erg s ^−1 , which is consistent with the X-ray cooling luminosity ( ${L}_{\mathrm{cool}}={1.9}_{-0.5}^{+0.2}\times {10}^{44}$ erg s ^−1 within r _cool = 43 kpc). These findings suggest that SPT0607 is a relaxed, cool-core cluster with AGN-regulated cooling at an epoch shortly after cluster formation, implying that the balance between cooling and feedback can be reached quickly. We discuss the implications for these findings on the evolution of AGN feedback in galaxy clusters. |
format |
Article in Journal/Newspaper |
author |
Megan Masterson Michael McDonald Behzad Ansarinejad Matthew Bayliss Bradford A. Benson Lindsey E. Bleem Michael S. Calzadilla Alastair C. Edge Benjamin Floyd Keunho J. Kim Gourav Khullar Taweewat Somboonpanyakul |
author_facet |
Megan Masterson Michael McDonald Behzad Ansarinejad Matthew Bayliss Bradford A. Benson Lindsey E. Bleem Michael S. Calzadilla Alastair C. Edge Benjamin Floyd Keunho J. Kim Gourav Khullar Taweewat Somboonpanyakul |
author_sort |
Megan Masterson |
title |
Evidence for AGN-regulated Cooling in Clusters at z ∼ 1.4: A Multiwavelength View of SPT-CL J0607-4448 |
title_short |
Evidence for AGN-regulated Cooling in Clusters at z ∼ 1.4: A Multiwavelength View of SPT-CL J0607-4448 |
title_full |
Evidence for AGN-regulated Cooling in Clusters at z ∼ 1.4: A Multiwavelength View of SPT-CL J0607-4448 |
title_fullStr |
Evidence for AGN-regulated Cooling in Clusters at z ∼ 1.4: A Multiwavelength View of SPT-CL J0607-4448 |
title_full_unstemmed |
Evidence for AGN-regulated Cooling in Clusters at z ∼ 1.4: A Multiwavelength View of SPT-CL J0607-4448 |
title_sort |
evidence for agn-regulated cooling in clusters at z ∼ 1.4: a multiwavelength view of spt-cl j0607-4448 |
publisher |
IOP Publishing |
publishDate |
2023 |
url |
https://doi.org/10.3847/1538-4357/acae9e https://doaj.org/article/43a3ed7fb69d400dbfbd03fa18d00080 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
The Astrophysical Journal, Vol 944, Iss 2, p 164 (2023) |
op_relation |
https://doi.org/10.3847/1538-4357/acae9e https://doaj.org/toc/1538-4357 doi:10.3847/1538-4357/acae9e 1538-4357 https://doaj.org/article/43a3ed7fb69d400dbfbd03fa18d00080 |
op_doi |
https://doi.org/10.3847/1538-4357/acae9e |
container_title |
The Astrophysical Journal |
container_volume |
944 |
container_issue |
2 |
container_start_page |
164 |
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1779320271267692544 |