A dataset provided by the European Space Agency

Name: The Physics of Cooling Flow Clusters with Central Radio Sources
Published: 2004-05-21T00:00:00Z

Proposal ID	014831
Title	The Physics of Cooling Flow Clusters with Central Radio Sources
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0148310101
DOI	https://doi.org/10.5270/esa-iigm0q5
Principal Investigator, PI	Dr Craig Sarazin
Abstract	Central galaxies in rich clusters are the sites of cluster cooling flows, withlarge masses of gas cooling through part of the X-ray band. Many of thesegalaxies host powerful radio sources. These sources can displace and compressthe X-ray gas leading to enhanced cooling and star formation. We proposeobservations of three bright cooling flows with radio sources that will exploitthe large collecting area and spectral resolution of XMM-Newton. We willconstrain the source of additional pressure in radio holes in the X-rayemission needed to support overlying shells of X-ray gas. We will address theproblem of the lack of kT < 1-2 keV gas in cooling flows by searching forabundance inhomogeneities, heating from the radio source, and excess absorption.
Publications	The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson M. G. Schroder A. C. et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos S. Saxton R. D. et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens Nicola Romer A. Kathy et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M The Axis Ratio Distribution of X-ray Clusters Observed by XMM-Newton \|Kawahara Hajime \| ApJ \| 719-1926 \| 2010 \| 2010ApJ...719.1926K \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...719.1926K A catalog of galaxy clusters observed by XMM-Newton \|Snowden S. L. Mushotzky R. F. et al. \| A&A \| 478-615 \| 2008 \| 2008A&A...478..615S \| http://ui.adsabs.harvard.edu/#abs/2008A&A...478..615S XMM-Newton and Chandra Observations of Abell 2626: Interacting Radio Jets and Cooling Core with Jet Precession? \|Wong Ka-Wah Sarazin Craig L. et al. \| ApJ \| 682-155 \| 2008 \| 2008ApJ...682..155W \| http://ui.adsabs.harvard.edu/#abs/2008ApJ...682..155W Constraints on turbulent velocity broadening for a sample of clusters groups and elliptical galaxies using XMM-Newton \|Sanders J. S. Fabian A. C. \| MNRAS \| 410-1797 \| 2011 \| 2011MNRAS.410.1797S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.410.1797S Revealing O VII from stacked X-ray grating spectra of clusters groups and elliptical galaxies \|Sanders J. S. Fabian A. C. \| MNRAS \| 412-35 \| 2011 \| 2011MNRAS.412L..35S \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.412L..35S An All-Sky Atlas of Radio/X-ray Associations \|Flesch E. \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies E. J. Romer A. Kathy et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc N. Sadibekova T. et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin Dacheng Webb Natalie A. \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page M. J. Brindle C. et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P A systematic cross-search for radio/infrared counterparts of XMM- Newton sources \|Combi J. A. Albacete Colombo J. F. et al. \| Ap&SS \| 331-53 \| 2011 \| 2011Ap&SS.331...53C \| http://ui.adsabs.harvard.edu/#abs/2011Ap&SS.331...53C Velocity width measurements of the coolest X-ray emitting material in the cores of clusters groups and elliptical galaxies \|Sanders J. S. Fabian A. C. \| MNRAS \| 429-2727 \| 2013 \| 2013MNRAS.429.2727S \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.429.2727S A Good Mass Proxy for Galaxy Clusters with XMM-Newton \|Zhao Hai-Hui Jia Shu-Mei et al. \| ApJ \| 778-124 \| 2013 \| 2013ApJ...778..124Z \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...778..124Z The diversity of quasars unified by accretion and orientation \|Shen Yue Ho Luis C. \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y Chemical Enrichment RGS cluster Sample (CHEERS): Constraints on turbulence \|Pinto Ciro Sanders Jeremy S. et al. \| A&A \| 575-38 \| 2015 \| 2015A&A...575A..38P \| http://ui.adsabs.harvard.edu/#abs/2015A&A...575A..38P Probing the evolution of the substructure frequency in galaxy clusters up to z ~ 1 \|Weissmann A. Bohringer H. \| A&A \| 555-147 \| 2013 \| 2013A&A...555A.147W \| http://ui.adsabs.harvard.edu/#abs/2013A&A...555A.147W Sunyaev-Zeldovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao Weike Chen Chen et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X Origin of central abundances in the hot intra-cluster medium. I. Individual and average abundance ratios from XMM-Newton EPIC \|Mernier F. de Plaa J. et al. \| A&A \| 592-157 \| 2016 \| 2016A&A...592A.157M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...592A.157M Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti F. Middei R. et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc N. Merloni A. et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Origin of central abundances in the hot intra-cluster medium. II. Chemical enrichment and supernova yield models \|Mernier F. de Plaa J. et al. \| A&A \| 595-126 \| 2016 \| 2016A&A...595A.126M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...595A.126M CHEERS: The chemical evolution RGS sample \|de Plaa J. Kaastra J. S. et al. \| A&A \| 607-98 \| 2017 \| 2017A&A...607A..98D \| http://ui.adsabs.harvard.edu/#abs/2017A&A...607A..98D Solar abundance ratios of the iron-peak elements in the Perseus cluster \|Hitomi Collaboration Aharonian Felix et al. \| Natur \| 551-478 \| 2017 \| 2017Natur.551..478H \| http://ui.adsabs.harvard.edu/#abs/2017Natur.551..478H Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas Konstantinos Reiprich Thomas H. \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M Mass-invariance of the iron enrichment in the hot haloes of massive ellipticals groups and clusters of galaxies \|Mernier F. de Plaa J. et al. \| MNRAS \| 478-116 \| 2018 \| 2018MNRAS.478L.116M \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.478L.116M The XMM Cluster Survey: Present status and latest results \|Viana P. T. P. Mehrtens N. et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V Solar chemical composition in the hot gas of cool-core ellipticals groups and clusters of galaxies \|Mernier F. Werner N. et al. \| MNRAS \| 480-95 \| 2018 \| 2018MNRAS.480L..95M \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.480L..95M The non-uniformity of galaxy cluster metallicity profiles \|Lovisari L. Reiprich T. H. \| MNRAS \| 483-540 \| 2019 \| 2019MNRAS.483..540L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483..540L Enrichment of the Hot Intracluster Medium: Observations \|Mernier F. Biffi V. et al. \| SSRv \| 214-129 \| 2018 \| 2018SSRv..214..129M \| http://ui.adsabs.harvard.edu/#abs/2018SSRv..214..129M Discovery of Dying Active Galactic Nucleus in Arp 187: Experience of Drastic Luminosity Decline within 104 yr \|Ichikawa Kohei Ueda Junko et al. \| ApJ \| 870-65 \| 2019 \| 2019ApJ...870...65I \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...870...65I Physical properties of the X-ray gas as a dynamical diagnosis for galaxy clusters \|Lagana T. F. Durret F. \| MNRAS \| 484-2807 \| 2019 \| 2019MNRAS.484.2807L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.484.2807L Searching for cool and cooling X-ray emitting gas in 45 galaxy clusters and groups \|Liu Haonan Pinto Ciro et al. \| MNRAS \| 485-1757 \| 2019 \| 2019MNRAS.485.1757L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.485.1757L Projected alignment of non-sphericities of stellar gas and dark matter distributions in galaxy clusters: analysis of the Horizon-AGN simulation \|Okabe Taizo Nishimichi Takahiro et al. \| MNRAS \| 478-1141 \| 2018 \| 2018MNRAS.478.1141O \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.478.1141O Testing emergent gravity on galaxy cluster scales \|Tamosiunas Andrius Bacon David et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood Devon L. Jeltema Tesla et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H The Y SZ Planck - Y SZ XMM scaling relation and its difference between cool-core and non-cool-core clusters \|Zhu Yue Wang Yuan-Hao et al. \| RAA \| 19-104 \| 2019 \| 2019RAA....19..104Z \| http://ui.adsabs.harvard.edu/#abs/2019RAA....19..104Z Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese A. Annis J. et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham Mona Clerc Nicolas et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba Matej Lieu Maggie et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc N. Kirkpatrick C. C. et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C The great Kite in the sky: A LOFAR observation of the radio source in Abell 2626 \|Ignesti A. Shimwell T. et al. \| A&A \| 643-172 \| 2020 \| 2020A&A...643A.172I \| http://ui.adsabs.harvard.edu/#abs/2020A&A...643A.172I The Metal Content of the Hot Atmospheres of Galaxy Groups \|Gastaldello Fabio Simionescu Aurora et al. \| Univ \| 7-208 \| 2021 \| 2021Univ....7..208G \| http://ui.adsabs.harvard.edu/#abs/2021Univ....7..208G Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z High-resolution X-ray spectroscopy of astrophysical plasmas with X-ray microcalorimeters \|Ezoe Yuichiro Ohashi Takaya \| RvMPP \| 5-4 \| 2021 \| 2021RvMPP...5....4E \| http://ui.adsabs.harvard.edu/#abs/2021RvMPP...5....4E The Planck clusters in the LOFAR sky. I. LoTSS-DR2: New detections and sample overview \|Botteon A. Shimwell T. W. et al. \| A&A \| 660-78 \| 2022 \| 2022A&A...660A..78B \| http://ui.adsabs.harvard.edu/#abs/2022A&A...660A..78B The Planck clusters in the LOFAR sky. III. LoTSS-DR2: Dynamic states and density fluctuations of the intracluster medium \|Zhang X. Simionescu A. et al. \| A&A \| 672-42 \| 2023 \| 2023A&A...672A..42Z \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..42Z The Planck clusters in the LOFAR sky. IV. LoTSS-DR2: Statistics of radio haloes and re-acceleration models \|Cassano R. Cuciti V. et al. \| A&A \| 672-43 \| 2023 \| 2023A&A...672A..43C \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..43C Outskirts of Abell 1795: Probing gas clumping in the intracluster medium \|Kovu00e1cs Orsolya Eszter Zhu Zhenlin et al. \| A&A \| 678-91 \| 2023 \| 2023A&A...678A..91K \| http://ui.adsabs.harvard.edu/#abs/2023A&A...678A..91K From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2002-12-28T01:49:55Z/2002-12-28T13:19:19Z
Version	17.56_20190403_1200
Mission Description	The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2004-05-21T00:00:00Z
Last Update	2025-01-27
Keywords	"excess absorption", "kev gas", "xmm newton", "additional pressure", "xray gas", "spectral resolution", "cluster cooling flows", "radio source", "xray emission", "radio sources", "xray band", "cooling flows", "enhanced cooling", "gas cooling", "bright cooling flows", "powerful radio sources", "XMM-Newton", "central galaxy", "abundance inhomogeneities", "rich cluster", "xray gas leading", "star formation", "central radio sources", "support overlying shells", "cooling flow cluster", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Craig Sarazin, 2004, 'The Physics of Cooling Flow Clusters with Central Radio Sources', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-iigm0q5