J/MNRAS/471/4990ivo://CDS.VizieR/J/MNRAS/471/4990doi:10.26093/cds/vizier.74714990CDSCaglar T.Hudaverdi M.2024-08-17T20:20:38Z2020-07-22T13:41:30ZCDS support team

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

cds-question@unistra.frgalaxy-clustersgalaxiesx-ray-sourcesIn this work, we studied 10 nearby (z<=0.038) galaxy clusters to understand possible interactions between hot plasma and member galaxies. A multi-band source detection was applied to detect point-like structures within the intra-cluster medium. We examined the spectral properties of a total of 391 X-ray point sources within each cluster's potential well. log N versus log S was studied in the energy range 2-10 keV to measure X-ray overdensities. Optical overdensities were also calculated to solve suppression/triggering phenomena for nearby galaxy clusters. X-ray and optical flux/luminosity properties (X/O, L_X_/L_B_ and L_X_/L_K_) were investigated for optically identified member galaxies. The X-ray luminosities of our point sources were found to be faint [40.08<=log(L_X_)<=42.39erg/s]. The luminosity range of point sources reveals possible contributions to X-ray emission from low-luminosity active galactic nuclei, X-ray binaries and star formation. We estimated ~2 times higher X-ray overdensities from galaxies within galaxy clusters compared to fields. Our results demonstrate that optical overdensities are much higher than X-ray overdensities at a cluster's centre, whereas X-ray overdensities increase through the outskirts of clusters. We conclude that high pressure from a cluster's centre affects the balance of galaxies and they lose a significant amount of their fuel. As a result, the clustering process quenches the X-ray emission of the member galaxies. We also find evidence that the existence of X-ray bright sources within a cluster environment can be explained by two main phenomena: contributions from off-nuclear sources and/or active galactic nucleus (AGN) triggering caused by galaxy interactions rather than AGN fuelling.2017MNRAS.471.4990Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/471/4990CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/xmm : XMM-Newton Observation Log (XMM-Newton Science Operation Center, 2012-)IX/55 : XMM-Newton Serendipitous Source Catalogue 3XMM-DR8 (XMM-SSC, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/471/4990https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/471/4990http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/471/4990https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/471/4990https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/471/4990http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/471/4990GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/471/4990/tablea1 (X-ray to optical properties of individual galaxies)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/471/4990/tablea1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/471/4990/tablea1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/471/4990/tablea1?GETtext/xml+votable180.050000true44.39028675.97696280.005555555555555556Cone search capability for table J/MNRAS/471/4990/tableb1 (Galaxy colour survey)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/471/4990/tableb1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/471/4990/tableb1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/471/4990/tableb1?GETtext/xml+votable180.050000true44.60256.04666670.005555555555555556Cone search capability for table J/MNRAS/471/4990/tableb2 (Properties of point sources studied in this work)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/471/4990/tableb2?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/471/4990/tableb2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/471/4990/tableb2?GETtext/xml+votable180.050000true44.60256.04666670.0055555555555555566/50 5607 5616 5618 8269 8271 18739 18742 18748 25669 25680 28249 28251 33469 33471 35055 43506 44554-445552.762881831355591e-19 3.3785437584409506e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/471/4990?format=asciiX-raydefaultJ/MNRAS/471/4990/tablea1X-ray to optical properties of individual galaxiesSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameGalaxy namemeta.id;meta.maincharzRedshift from NASA/IPAC Extragalactic Database Astronomical Databasesrc.redshiftdoubleRmag? R-band magnitude from the Vizier databasemagphot.mag;em.opt.RfloatnullableFX/FO? X-ray to optical flux ratiophot.flux;arith.ratiofloatnullableBmagApparent blue magnitude from Vizier data basemagphot.mag;em.opt.BfloatKmag? Apparent K magnitude from Tully (2015, Cat. J/AJ/149/171) and Dalya et al. (2016, Cat. VII/275)magphot.mag;em.IR.KfloatnullablelogLXHard band logarithmic X-ray luminosity from spectral analysislog(1e-07W)phys.luminosity;em.X-rayfloatlogLK? K-band luminosity calculated from extinction corrected K-band magnitudelog(solLum)phys.luminosity;em.IRfloatnullablelogLBLogarithmic blue optical luminosity calculated from extinction corrected B-band magnitudelog(solLum)phys.luminosity;em.opt.BfloatMTypeMorphological type of galaxysrc.morph.typecharClusterName of cluster host for identified galaxiesmeta.id.parentchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainJ/MNRAS/471/4990/tableb1Galaxy colour surveyrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSource name, XMMU JHHMMSS.s+DDMMSSmeta.id;meta.maincharHRHardness ratio (1)phot.flux;arith.ratiofloate_HRHardness ratio error (1)stat.errorfloatlogFXLogarithmic X-ray fluxlog(mW.m**-2)phot.flux;em.X-rayfloatlogLXLogarithmic X-ray luminositylog(1e-07W)phys.luminosity;em.X-rayfloatrmagr-band magnitudemagphot.mag;em.opt.Rfloatg-rg-r/b-r colour indexmagphot.color;em.opt.B;em.opt.RfloatDistProjected distance from the centre of the related galaxy clusterMpcpos.distancefloatPLikelihood of optical association%stat.likelihoodintTypeGalaxy type in coloursrc.classcharClusterCluster namemeta.id.parentchar_RAPosition from Name (right ascension part)degpos.eq.ra;meta.main_DEPosition from Name (declination part)degpos.eq.dec;meta.mainJ/MNRAS/471/4990/tableb2Properties of point sources studied in this workrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameObject name, XMMU JHHMMSS.s+DDMMSSmeta.id;meta.maincharNCountNet countctphot.count;em.X-rayintLogFXLogarithmic X-ray fluxlog(mW.m**-2)phot.flux;em.X-rayfloatlogLXLogarithmic X-ray luminositylog(1e-07W)phys.luminosity;em.X-rayfloatClusterCluster namemeta.id.parentcharOptCTPOptical counterpartmeta.id.assoccharz? Redshiftsrc.redshiftdoublenullable_RAPosition from Name (right ascension part)degpos.eq.ra;meta.main_DEPosition from Name (declination part)degpos.eq.dec;meta.main