VII/96ivo://CDS.VizieR/VII/96CDSSTRUBLE M.F.ROOD H.J.1997-12-09T22:25:56Z1997-12-09T23:25:45ZCDS support team

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

cds-question@unistra.frgalaxy-clustersgalaxy-classification-systemsA catalog is presented which contains Rood-Sastry (1971, hereafter RS) morphological types for all 2712 Abell clusters.1987ApJS...63..555Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/VII/96CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=VII/96https://vizier.iucaa.in/viz-bin/VizieR-2?-source=VII/96http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=VII/96https://vizier.cds.unistra.fr/viz-bin/votable?-source=VII/96https://vizier.iucaa.in/viz-bin/votable?-source=VII/96http://vizieridia.saao.ac.za/viz-bin/votable?-source=VII/96GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultVII/96/table1Catalog of morphological properties of Abell clustersrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAbellAbell cluster identificationmeta.id;meta.mainintn_Abell[*] An '*' indicates that the cluster is not in Abell's (1980) statistical samplemeta.notecharDistDistance class as given by Abell (1980)src.class.distanceintnGalAbell's (1980) number count of galaxiesmeta.numberintRadiusRadius of the circular observation window which our data were obtained (1mm=67.14")mmphys.angSize;srcintRS1Basic RS type (1)src.classcharRS2Subsidiary property of RS type (2)src.classcharRS3[]? Number of bright galaxies used to determine RS type for both the C and L typesmeta.numberintT1First brightest cluster galaxy Hubble typesrc.morph.typecharSep1a[]? Separation, see note (3)mmpos;arith.difffloatSep1b[]? Separation, see note (3)mmpos;arith.difffloatT2Second brightest cluster galaxy Hubble typesrc.morph.typecharSep2a[]? Separation, see note (3)mmpos;arith.difffloatSep2b[]? Separation, see note (3)mmpos;arith.difffloatT3Third brightest cluster galaxy Hubble typesrc.morph.typecharSep3a[]? Separation, see note (3)mmpos;arith.difffloatSep3b[]? Separation, see note (3)mmpos;arith.difffloatr12Separation between the first and second most luminous cluster galaxies (1mm=67.14")mmpos;arith.difffloatr13Separation between the first and third most luminous cluster galaxies (1mm=67.14")mmpos;arith.difffloatr23Separation between the second and third most luminous cluster galaxies (1mm=67.14")mmpos;arith.difffloatNb[]? Number of apparent double galaxies not among the three most luminous cluster galaxiesmeta.numberintNt[]? Number of apparent triple galaxies not among the three most luminous cluster galaxiesmeta.numberintn_Nt[n] A 'n' indicates that a galaxy with a multiple nucleus is observed in the clustermeta.notecharFRS1aBasic RS type for the first subcluster in an F cluster (1)meta.notecharFRS1bSubsidiary property of RS type of FRS1 (2)meta.notecharFRS1c[]? Number of bright galaxies used to determine FRS1 RS type for both the C and L typesmeta.numberintFRS2aBasic RS type for the second subcluster in an F cluster (1)meta.notecharFRS2bSubsidiary property of RS type of FRS2 (2)meta.notecharFRS2c[]? Number of bright galaxies used to determine FRS2 RS type for both the C and L typesmeta.numberintFRS3aBasic RS type for the third subcluster in an F cluster (1)meta.notecharF3RS3bSubsidiary property of RS type of FRS3 (2)src.classcharF3RS3c[]? Number of bright galaxies used to determine FRS3 RS type for both the C and L typesmeta.numberintOtherOther source data (4)meta.idcharVII/96/table2Additional data for resolved F clustersComComments (4)meta.notecharRS1Basic RS type for the first subclustersrc.classcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAbellAbell cluster identificationmeta.id;meta.mainintu_Abell[:] Uncertainty flag on F type of the cluster (RS1 in table1)meta.code.errorcharm_Abell[EWNSM] Component of the cluster (1)meta.code.multipcharRSBasic revised RS typesrc.classcharT1First brightest cluster galaxy Hubble typesrc.morph.typecharSepT1a[]? Separation, see note (2)mmpos;arith.difffloatSepT1b[]? Separation, see note (2)mmpos;arith.difffloatT2Second brightest cluster galaxy Hubble typesrc.morph.typecharSepT2a[]? Separation, see note (2)mmpos;arith.difffloatSepT2b[]? Separation, see note (2)mmpos;arith.difffloatT3Third brightest cluster galaxy Hubble typesrc.morph.typecharSepT3a[]? Separation, see note (2)mmpos;arith.difffloatSepT3b[]? Separation, see note (2)mmpos;arith.difffloatr12Separation between the first and second most luminous cluster galaxies (1mm=67.14")mmpos;arith.difffloatr13Separation between the first and third most luminous cluster galaxies (1mm=67.14")mmpos;arith.difffloatr23Separation between the second and third most luminous cluster galaxies (1mm=67.14")mmpos;arith.difffloatNb[]? Number of apparent galaxies that are not among the three most luminous cluster galaxiesmeta.numberintNt[]? Number of apparent triple galaxies not among the three most luminous cluster galaxiesmeta.numberintRS2Subsidiary property of RS type (3)src.classcharRS3[]? Number of bright galaxies used to determine FRS1 RS type for both the C and L typesmeta.numberintSep[]? Separation of the components (1mm=67.14")mmpos;arith.difffloatm_Sep[SENWM] Component designationmeta.code.multipcharPA[]? Position angle of the separation vector of the componentsdegpos.posAngintn_PA[SENWM] Component designationmeta.notecharVII/96/table3Additional data for Abell clusters with non-cluster populationComComments (4)meta.notecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAbellAbell numbermeta.id;meta.mainintu_AbellUncertainty flag on the type of the clustermeta.code.errorcharn_Abell[CX] C: confused, X: probable cluster in the foreground of an Abell clustermeta.notecharRS1Basic RS type (1)src.classcharRS2Subsidiary property of RS type (2)src.classcharRS3[]? Number of bright galaxies used to determine RS type for both the C and L typesmeta.numberintT1First brightest cluster galaxy Hubble typesrc.morph.typecharSepT1a[]? Separation, see note (3)pos;arith.difffloatT2Second brightest cluster galaxy Hubble typesrc.morph.typecharSepT2a[]? Separation, see note (3)pos;arith.difffloatT3Third brightest cluster galaxy Hubble typesrc.morph.typecharSepT3a[]? Separation, see note (3)pos;arith.difffloatSepT3b[]? Separation, see note (3)pos;arith.difffloatr12Separation between the first and second most luminous cluster galaxies (1mm=67.14")pos;arith.difffloatr13Separation between the first and third most luminous cluster galaxies (1mm=67.14")pos;arith.difffloatr23Separation between the second and third most luminous cluster galaxies (1mm=67.14")pos;arith.difffloatNb[]? Number of apparent galaxies that are not among the three most luminous cluster galaxiesmeta.numberintFRS1aRevised RS type for the first subclustermeta.notecharFRS1c[]? Number of bright galaxies used to determine FRS1 RS type for both the C and L typesmeta.numberintFRS2aRevised RS type for the second subclustermeta.notecharFRS2c[]? Number of bright galaxies used to determine FRS2 RS type for both the C and L typesmeta.numberint