A dataset provided by the European Space Agency

Name: Nature of the cool component in the cD Cluster AWM7
Published: 2004-08-22T00:00:00Z

Proposal ID	013595
Title	Nature of the cool component in the cD Cluster AWM7
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0135950301
DOI	https://doi.org/10.5270/esa-0yz4iy1
Principal Investigator, PI	Dr Tae Furusho
Abstract	AWM7 is the 2nd brightest poor cluster of galaxies (with kT \le 4 keV) in thesky next to the Centaurus cluster. Based on the spatially resolved spectra ofthe central cool component, we can unambiguously determine the origin of thecool component and look into its evolution process in the cD type clusters. Thecool component of AWM7 is extended and is probably in an early stage ofevolution, placing this cluster an important target for the systematic study ofthe cool-component evolution. The proposed 30 ks observation will also enable usto examine non-uniformity in the spatial distribution of metals, and further toestimate the cusp structure of the gravitational potential which confines thehot-component gas.
Publications	Metal abundances in the cool cores of galaxy clusters \|de Grandi, S., Molendi, S., \| A&A \| 508-565 \| 2009 \| 2009A&A...508..565D \| http://ui.adsabs.harvard.edu/#abs/2009A&A...508..565D Radial profiles of Fe abundance in the intracluster medium of nearby clusters observed with XMM-Newton \|Matsushita, K., \| A&A \| 527-134 \| 2011 \| 2011A&A...527A.134M \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.134M 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 Deep Chandra and XMM-Newton X-ray observations of AWM 7 - I. Investigating X-ray surface brightness fluctuations \|Sanders, J. S., Fabian, A. C., \| MNRAS \| 421-726 \| 2012 \| 2012MNRAS.421..726S \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.421..726S 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 2XMM ultraluminous X-ray source candidates in nearby galaxies \|Walton, D. J., Roberts, T. P., et al. \| MNRAS \| 416-1844 \| 2011 \| 2011MNRAS.416.1844W \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.416.1844W 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 Oxygen Abundances in the Milky Way Using X-Ray Absorption Measurements toward Galaxy Clusters \|Baumgartner, W. H., Mushotzky, R. F., \| ApJ \| 639-929 \| 2006 \| 2006ApJ...639..929B \| http://ui.adsabs.harvard.edu/#abs/2006ApJ...639..929B Cold fronts in galaxy clusters \|Ghizzardi, S., Rossetti, M., \| A&A \| 516-32 \| 2010 \| 2010A&A...516A..32G \| http://ui.adsabs.harvard.edu/#abs/2010A&A...516A..32G A large catalogue of ultraluminous X-ray source candidates in nearby galaxies \|Walton, D. J., Gladstone, J. C., et al. \| AN \| 332-354 \| 2011 \| 2011AN....332..354W \| http://ui.adsabs.harvard.edu/#abs/2011AN....332..354W 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 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 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 Detection of an Unidentified Emission Line in the Stacked X-Ray Spectrum of Galaxy Clusters \|Bulbul, Esra, Markevitch, Maxim, et al. \| ApJ \| 789-13 \| 2014 \| 2014ApJ...789...13B \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...789...13B 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 Sunyaev-Zel.dovich 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 Where do the 3.5 keV photons come from? A morphological study of the Galactic Center and of Perseus \|Carlson, Eric, Jeltema, Tesla, \| JCAP \| 2-9 \| 2015 \| 2015JCAP...02..009C \| http://ui.adsabs.harvard.edu/#abs/2015JCAP...02..009C A novel scenario for the possible X-ray line feature at virgul3.5 keV. Charge exchange with bare sulfur ions \|Gu, L., Kaastra, J., et al. \| A&A \| 584-11 \| 2015 \| 2015A&A...584L..11G \| http://ui.adsabs.harvard.edu/#abs/2015A&A...584L..11G 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 Suzaku Observations of AWM 7 Cluster of Galaxies: Temperatures, Abundances, and Bulk Motions \|Sato, Kosuke, Matsushita, Kyoko, et al. \| PASJ \| 60-333 \| 2008 \| 2008PASJ...60S.333S \| http://ui.adsabs.harvard.edu/#abs/2008PASJ...60S.333S AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda, J., Guainazzi, M., \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S X-Ray Morphological Analysis of the Planck ESZ Clusters \|Lovisari, Lorenzo, Forman, William R., et al. \| ApJ \| 846-51 \| 2017 \| 2017ApJ...846...51L \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...846...51L 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 X-Ray Lines from Dark Matter Annihilation at the keV Scale \|Brdar, Vedran, Kopp, Joachim, et al. \| PhRvL \| 120-61301 \| 2018 \| 2018PhRvL.120f1301B \| http://ui.adsabs.harvard.edu/#abs/2018PhRvL.120f1301B 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 WIMP dark matter candidates and searches---current status and future prospects \|Roszkowski, Leszek, Sessolo, Enrico Maria, \| RPPh \| 81-66201 \| 2018 \| 2018RPPh...81f6201R \| http://ui.adsabs.harvard.edu/#abs/2018RPPh...81f6201R Resonantly Produced 7A keV Sterile Neutrino Dark Matter Models and the Properties of Milky Way Satellites \|Abazajian, Kevork N., \| PhRvL \| 112-161303 \| 2014 \| 2014PhRvL.112p1303A \| http://ui.adsabs.harvard.edu/#abs/2014PhRvL.112p1303A 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 Laboratory Measurements of X-Ray Emission from Highly Charged Argon Ions \|Bulbul, Esra, Foster, Adam, et al. \| ApJ \| 870-21 \| 2019 \| 2019ApJ...870...21B \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...870...21B 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 Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton \|Lovisari, Lorenzo, Schellenberger, Gerrit, et al. \| ApJ \| 892-102 \| 2020 \| 2020ApJ...892..102L \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...892..102L Comparing different mass estimators for a large subsample of the Planck-ESZ clusters \|Lovisari, L., Ettori, S., et al. \| A&A \| 644-78 \| 2020 \| 2020A&A...644A..78L \| http://ui.adsabs.harvard.edu/#abs/2020A&A...644A..78L Metastable conformal dark matter \|Brax, Philippe, Kaneta, Kunio, et al. \| PhRvD \| 103-115016 \| 2021 \| 2021PhRvD.103k5016B \| http://ui.adsabs.harvard.edu/#abs/2021PhRvD.103k5016B 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 A Search for the 3.5 keV Line from the Milky Way.s Dark Matter Halo with HaloSat \|Silich, E. 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The Perseus-Pisces supercluster and the Southern Great Wall as traced by X-ray luminous galaxy clusters \|B\\u00f6hringer, Hans, Chon, Gayoung, \| A&A \| 651-16 \| 2021 \| 2021A&A...651A..16B \| http://ui.adsabs.harvard.edu/#abs/2021A&A...651A..16B Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters \|Wicker, R., Douspis, M., et al. \| A&A \| 674-48 \| 2023 \| 2023A&A...674A..48W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...674A..48W O, Ne, Mg, and Fe Abundances in Hot X-Ray-emitting Halos of Galaxy Clusters, Groups, and Giant Early-type Galaxies with XMM-Newton RGS Spectroscopy \|Fukushima, Kotaro, Kobayashi, Shogo B., \| ApJ \| 953-112 \| 2023 \| 2023ApJ...953..112F \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...953..112F Outskirts of Abell 1795: Probing gas clumping in the intracluster medium \|Kov\\u00e1cs, 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 Was There a 3.5 keV Line? \|Dessert, Christopher, Foster, Joshua W., et al. \| ApJ \| 964-185 \| 2024 \| 2024ApJ...964..185D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...964..185D 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	2003-02-02T09:24:15Z/2003-02-02T18:15:58Z
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	2004-08-22T00:00:00Z
Keywords	"gravitational potential", "cool component evolution", "hot component gas", "cd type clusters", "spatial distribution", "resolved spectra", "cd cluster awm7", "cool component", "cusp structure", "centaurus cluster", "central cool component", "evolution process"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Tae Furusho, 2004, 'Nature of the cool component in the cD Cluster AWM7', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0yz4iy1