J/AJ/160/103ivo://CDS.VizieR/J/AJ/160/103doi:10.26093/cds/vizier.51600103CDSPrasow-Emond M.Hlavacek-Larrondo J.Rhea C.L.Latulippe M.Gendron-Marsolais M.-L.Richard-Laferriere A.Sanders J.S.Edge A.C.Allen S.W.,Mantz A.von der Linden A.2021-02-19T07:51:01Z2020-11-05T12:10:05ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxy-clustersblack-holesradio-spectroscopyx-ray-sourceschemical-abundancesredshiftedClusters of galaxies are outstanding laboratories for understanding the physics of supermassive black hole (SMBH) feedback. Here we present the first Chandra, Karl G. Jansky Very Large Array, and Hubble Space Telescope analysis of MACS J1447.4+0827 (z=0.3755), one of the strongest cool core clusters known, in which extreme feedback from its central SMBH is needed to prevent the hot intracluster gas from cooling. Using this multiwavelength approach, including 70ks of Chandra X-ray observations, we detect the presence of collimated jetted outflows that coincide with a southern and a northern X-ray cavity. The total mechanical power associated with these outflows (P_cav_~6x1044erg/s) is roughly consistent with the energy required to prevent catastrophic cooling of the hot intracluster gas (L_cool_=1.71{+/-}0.01x1045erg/s for t_cool_=7.7Gyr), implying that powerful SMBH feedback was in place several Gyr ago in MACS J1447.7+0827. In addition, we detect the presence of a radio minihalo that extends over 300kpc in diameter (P1.4GHz=3.0{+/-}0.3x1024W/Hz). The X-ray observations also reveal an ~20kpc plumelike structure that coincides with optical dusty filaments that surround the central galaxy. Overall, this study demonstrates that the various physical phenomena occurring in the most nearby clusters of galaxies are also occurring in their more distant analogs.2020AJ....160..103Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/160/103CatalogResearchIsServedByTAP VizieR generic servicerelated-toI/221 : The Magellanic Catalogue of Stars - MACS (Tucholke+ 1996)VIII/76 : Leiden/Argentine/Bonn (LAB) Survey of Galactic HI (Kalberla+, 2005)J/A+A/495/231 : Multiwavelength study of Cyg OB2 5 (Linder+, 2009)J/ApJ/690/295 : Chandra obs. of J1604+4314 supercluster (Kocevski+, 2009)J/ApJ/729/22 : SEDs of galaxy cluster members (Atlee+, 2011)J/other/Ap/54.147 : Study of 230 IRAS-FSC galaxies (Hovhannisyan+, 2011)J/ApJ/756/139 : Spectro. redshifts of galaxies in groups (Connelly+, 2012)J/MNRAS/425/1215 : Multiwavelength survey of AGNs (Klesman+, 2012)J/ApJ/774/23 : Chandra observations of SPT-SZ clusters (McDonald+, 2013)J/ApJ/799/60 : X-ray galaxy clusters in the CFHTLS fields (Mirkazemi+,2015)J/ApJ/813/77 : Galaxy clust.: radio halos, relics & parameters (Yuan+,2015)J/MNRAS/453/1201 : Radio properties of brightest cluster galaxies (Hogan+,2015)J/A+A/622/A22 : Abell 1914 multiwavelength radio images (Mandal+, 2019)J/ApJS/247/25 : The SPTpol Extended Cluster Survey (Bleem+, 2020)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/160/103https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/160/103http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/160/103https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/160/103https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/160/103http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/160/103GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapX-rayMillimeterRadiodefaultJ/AJ/160/103/fig7PropertiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRad[20.5/283] Radiuskpcphys.size.radiusdoublee_Rad[3.05/52.5] Lower uncertainty in Radkpcstat.errordoubleE_Rad[5.81/52.5] Upper uncertainty in Radkpcstat.error;stat.maxdoubleTe[4.39/9.18] Electronic temperaturekeVphys.temperaturedoublee_Te[0.25/0.86] Lower uncertainty in TekeVstat.errordoubleE_Te[0.25/0.86] Upper uncertainty in TekeVstat.error;stat.maxdoubleTeDep[4.02/7.02]? Deprojected electronic temperaturekeVphys.temperature;phys.electronfloatnullablee_TeDep[0.12/0.82]? Lower uncertainty in TeDepkeVstat.errorfloatnullableE_TeDep[0.12/0.83]? Upper uncertainty in TeDepkeVstat.error;stat.maxfloatnullableAbd[0.15/0.58] Abundance relative to solarlog(Sun)phys.abunddoublee_Abd[0.03/0.19] Lower uncertainty in Abdlog(Sun)stat.errordoubleE_Abd[0.03/0.19] Upper uncertainty in Abdlog(Sun)stat.error;stat.maxdoubleAbdDep[0.15/0.58] Deprojected abundance relative to solarlog(Sun)phys.abundfloate_AbdDep[0.03/0.19] Lower uncertainty in AbdDeplog(Sun)stat.errorfloatE_AbdDep[0.03/0.19] Upper uncertainty in AbdDeplog(Sun)stat.error;stat.maxfloatPe[6.4e-11/1.8e-9] Electron pressure; erg/cm31e-07J.cm**-3phys.electrondoublee_Pe[1.2e-12/1.9e-11] Lower uncertainty in Pe1e-07J.cm**-3stat.errordoubleE_Pe[1.2e-12/1.9e-11] Upper uncertainty in Pe1e-07J.cm**-3stat.error;stat.maxdoublePeDep[1.6e-10/1.7e-9] Deprojected electron pressure; erg/cm31e-07J.cm**-3phys.electrondoublee_PeDep[3.2e-15/5.2e-13] Lower uncertainty in PeDep1e-07J.cm**-3stat.errordoubleE_PeDep[3e-15/5.1e-13] Upper uncertainty in PeDep1e-07J.cm**-3stat.error;stat.maxdoubleNe[0.002/0.12] Electron densitycm**-3phys.density;phys.electrondoublee_Ne[0.0004/0.3] Lower uncertainty in Necm**-3stat.errordoubleE_Ne[0.0004/0.03] Upper uncertainty in Necm**-3stat.error;stat.maxdoubleNeDep[0.003/0.1] Electron densitycm**-3phys.densitydoublee_NeDep[0.0005/0.02] Uncertainty in NeDepcm**-3stat.errordoubleJ/AJ/160/103/fig8Average cooling time profilesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRadAccACCEPT radius (1)kpcphys.size.radiusdoubleTcAccACCEPT cooling time (1)Gyrtime.agedoubleRadSPT? SPT survey average radius (2)kpcphys.size.radius;stat.meandoublenullableTcSPT? SPT survey average cooling time (2)Gyrtime.agedoublenullablee_TcSPT? Lower uncertainty in TcSPT (2)Gyrstat.errordoublenullableE_TcSPT? Upper uncertainty in TcSPT (2)Gyrstat.error;stat.maxdoublenullableRadPhx? Phoenix survey radius (3)kpcphys.size.radiusdoublenullableTcPhx? Phoenix survey radius (3)Gyrtime.agedoublenullableRadMS1447? MACS J1447.4+0827 radiuskpcphys.size.radiusdoublenullablee_RadMS1447? Lower uncertainty in RadMS1447kpcstat.errordoublenullableE_RadMS1447? Upper uncertainty in RadMS1447kpcstat.error;stat.maxdoublenullableTcMS1447? MACS J1447.4+0827 cooling timeGyrtime.agefloatnullablee_TcMS1447? Lower uncertainty in TcRMS1447Gyrstat.errordoublenullableE_TcMS1447? Upper uncertainty in TcRMS1447Gyrstat.error;stat.maxdoublenullableJ/AJ/160/103/fig10Radio spectral energy distributionrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintFreq[0.15/19] FrequencyGHzem.wlfloatFlux[8/64] Flux densitymJyphot.fluxfloate_Flux[0.2/9.9] Uncertainty in FluxmJystat.error;phot.fluxfloatFreqMH[1.4]? Mini-Halo frequencyGHzem.wlfloatnullableFluxMH[5.7]? Mini-Halo flux densitymJyphot.fluxfloatnullablee_FluxMH[0.5]? Uncertainty in FluxMHmJystat.errorfloatnullableJ/AJ/160/103/fig11X-ray luminositiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLxSpt[0.35/16.8]? SPT survey 0.1-2.4 keV luminosity (1e44erg/s) (1)1e+37Wphys.luminosity;em.X-rayfloatnullablee_LxSpt[0.1/1.5]? Uncertainty in LxSpt (1)1e+37Wstat.errorfloatnullablezSpt[0.2/1.48]? SPT survey redshift (1)src.redshift;pos.heliocentricfloatnullableLxMACS[4.1/42.2]? MACS survey 0.1-2.4 keV luminosity (1e44erg/s) (2)1e+37Wphys.luminosity;em.X-rayfloatnullablezMACS[0.3/0.7]? MACS survey redshift (2)src.redshift;pos.heliocentricfloatnullablee_LxMACS[0.2/1.5]? Uncertainty in LxMACS (2)1e+37Wstat.errorfloatnullablezPlanck[0.04/0.45] Planck survey redshift (3)src.redshift;pos.heliocentricfloatLxPlanck[0.92/26.4] Planck survey 0.1-2.4 keV luminosity (1e44erg/s) (3)1e+37Wphys.luminosity;em.X-rayfloate_LxPlanck[0.01/0.38] Uncertainty in LxPlanck (3)1e+37Wstat.errorfloatLxPhx? Phoenix survey 0.1-2.4 keV luminosity (1e44erg/s) (4)1e+37Wphys.luminosity;em.X-rayfloatnullablee_LxPhx? Uncertainty in LxPhx (4)1e+37Wstat.errorfloatnullablezPhx? Phoenix survey redshift (4)src.redshift;pos.heliocentricfloatnullablezM1447? MACS J1447.4+0827 redshiftsrc.redshift;pos.heliocentricfloatnullableLxM1447? MACS J1447.4+0827 0.1-2.4 keV luminosity (1e44erg/s)1e+37Wphys.luminosity;em.X-rayfloatnullablee_LxM1447? Uncertainty in LxM14471e+37Wstat.errorfloatnullableJ/AJ/160/103/fig12Cooling luminositiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzHL[0.01/0.55] Redshift (1)src.redshift;pos.heliocentricdoublelogTcHL[43.7/45.5] log cooling luminosity; erg/s (1)log(1e-07W)phys.luminositydoublez? MACS J1447.4+0827 redshiftsrc.redshift;pos.heliocentricfloatnullablelogTc? Log MACS J1447.4+0827 cooling luminosity (erg/s)log(1e-07W)phys.luminositydoublenullablezPhx? Phoenix survey redshift (2)src.redshift;pos.heliocentricdoublenullablelogTcPhx? log Phoenix survey cooling luminosity (erg/s) (2)log(1e-07W)phys.luminositydoublenullableJ/AJ/160/103/fig13Total mechanical power of the X-ray cavities as a function of the cooling luminosity at 7.7GyrsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLcNu? Cooling luminosity from Nulsen+, 2009AIPC.1201..198N (1)1e+35Wphys.luminositydoublenullablePcavNu? Cavity power from Nulsen+, 2009AIPC.1201..198N (1e42erg/s)1e+35Wphys.luminositydoublenullablee_LcNu? Lower uncertainty in LcNu1e+35Wstat.errordoublenullableE_LcNu? Upper uncertainty in LcNu1e+35Wstat.error;stat.maxdoublenullablee_PcavNu? Lower uncertainty in PcavNu1e+35Wstat.errordoublenullableE_PcavNu? Upper uncertainty in PcavNu1e+35Wstat.error;stat.maxdoublenullableLcDu? Cooling luminosity from Dunn+, 2008MNRAS.385..757D (1)1e+35Wphys.luminosityintnullablePcavDu? Cavity power from Dunn+, 2008MNRAS.385..757D (1e42erg/s)1e+35Wphys.luminosityintnullablee_PcavDu? Lower uncertainty in PcavDu1e+35Wstat.errorintnullableE_PcavDu? Upper uncertainty in PcavDu1e+35Wstat.error;stat.maxintnullableLc? MACS J1447.4+0827 cooling luminosity (1)1e+35Wphys.luminosityintnullablePcav? MACS J1447.4+0827 cavity power (1e42erg/s)1e+35Wphys.luminosityintnullableLcPhx? Cooling luminosity from from Phoenix, McDonald+, 2019ApJ...885...63M (1)1e+35Wphys.luminosityfloatnullablePcavPhx? Cavity power from Phoenix, McDonald+, 2019ApJ...885...63M (1e42erg/s)1e+35Wphys.luminosityfloatnullablee_PcavPhx? Uncertainty in PcavPhx1e+35Wstat.errorintnullableLcHL15? Cooling luminosity from Hlavacek-Larrondo+, 2015ApJ...805...35H (1)1e+35Wphys.luminosityintnullablePcavHL15? Cavity power from Hlavacek-Larrondo+, 2015ApJ...805...35H (1e42erg/s)1e+35Wphys.luminosityintnullablee_PcavHL15? Uncertainty in PcavHL151e+35Wstat.errordoublenullableLcHL12? Cooling luminosity from Hlavacek-Larrondo+, 2012MNRAS.424..224H (1)1e+35Wphys.luminosityintnullablePcavHL12? Cavity power from Hlavacek-Larrondo+, 2012MNRAS.424..224H (1e42erg/s)1e+35Wphys.luminosityfloatnullableLcRACooling luminosity from Rafferty+, 2006ApJ...652..216R (1)1e+35Wphys.luminosityfloatPcavRACavity power from Rafferty+, 2006ApJ...652..216R (1e42erg/s)1e+35Wphys.luminosityfloate_PcavRALower uncertainty in PcavRA1e+35Wstat.errorfloatE_PcavRAUpper uncertainty in PcavRA1e+35Wstat.error;stat.maxfloat