J/A+A/361/863ivo://CDS.VizieR/J/A+A/361/863doi:10.26093/cds/vizier.33610863CDSGavazzi G.Franzetti P.Boselli A.Pierini D.Scodeggio M.2000-10-14T23:21:54Z2000-10-14T23:21:48ZCDS support team

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

cds-question@unistra.frgalaxiesphotometrysurface-photometrygalaxy-classification-systemsinfrared-photometryWe present near-infrared H-band (1.65{mu}m) surface brightness profile decomposition for 1157 galaxies in five nearby clusters of galaxies: Coma, A1367, Virgo, A262 and Cancer, and in the bridge between Coma and A1367 in the "Great Wall". The optically selected (m_pg_<=16.0) sample is representative of all Hubble types, from E to Irr+BCD, except dE and of significantly different environments, spanning from isolated regions to rich clusters of galaxies. We model the surface brightness profiles with a de Vaucouleurs r^1/4^ law (dV), with an exponential disk law (E), or with a combination of the two (B+D). From the fitted quantities we derive the H band effective surface brightness ({mu}_e_) and radius (r_e_) of each component, the asymptotic magnitude H_T_ and the light concentration index C_31_. We find that: i) Less than 50% of the Elliptical galaxies have pure dV profiles. The majority of E to Sb galaxies is best represented by a B+D profile. All Scd to BCD galaxies have pure exponential profiles. ii) The type of decomposition is a strong function of the total H band luminosity (mass), independent of the Hubble classification: the fraction of pure exponential decompositions decreases with increasing luminosity, that of B+D increases with luminosity. Pure dV profiles are absent in the low luminosity range L_H_<10^10^L_{sun}_ and become dominant above 10^11^L_{sun}_.2000A&A...361..863Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/361/863CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/120/489 : Galaxies morphology and IR photometry I. (Gavazzi+ 1996)J/A+AS/120/521 : Galaxies morphology and IR photometry II. (Gavazzi+ 1996)J/A+AS/142/65 : Galaxies morphology and IR photometry III. (Gavazzi+ 2000)J/A+AS/142/73 : Galaxies morphology and IR photometry IV. (Boselli+ 2000)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/361/863https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/361/863http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/361/863https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/361/863https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/361/863http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/361/863GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticalInfrareddefaultJ/A+A/361/863/table2Photometric parameters of the target galaxiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameCGCG (Zwicky et al., 1961-68, <VII/190>) or VCC (Binggeli et al., 1985AJ.....90.1681B)meta.id;meta.maincharm_Name[NSWEC] Multiplicity index on Namemeta.code.multipcharMTypeMorphological type (Binggeli et al., 1985AJ.....90.1681B)src.morph.typecharAggAggregation parameter - cluster membershipmeta.code.membercharDistDistanceMpcpos.distancefloatFilter[HK] Infrared filtermeta.code;instr.filtercharDTypeDecomposition type (1)meta.notecharDTypeBDecomposition type of bulge (1)meta.notecharrebf? Effective radius of the bulgearcsecphys.angSize;srcfloatnullablemuebf? Effective surface brightness of bulgemag.arcsec**-2phot.mag.sbfloatnullableredf? Effective radius of the diskarcsecphys.angSize;srcfloatnullablemuedf? Effective surface brightness of diskmag.arcsec**-2phot.mag.sbfloatnullablereEmpirical effective radiusarcsecphys.angSize;srcfloatmueEmpirical effective surface brightnessmag.arcsec**-2phot.mag.sbfloatHTTotal magnitude integrated to infinitymagphot.mag;em.IR.HfloatC31? Concentration indexphys.size;arith.ratiofloatnullableB/T? Bulge to total flux ratiophot.flux.sb;arith.ratiofloatnullablerB(25)Optical isophotal diameter (at 25mag/arcsec+2)arcminphys.angSize;srcfloatrH(20.5)NIR isophotal radius (at 20.5mag/arcsec+2)arcsecphys.angSize;srcfloat