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<ri:Resource created="2006-03-21T21:10:00Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Galaxies morphology and IR photometry. VIII</title><shortName>J/MNRAS/332/422</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/332/422</identifier><altIdentifier>doi:10.26093/cds/vizier.73320422</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pierini D.</name></creator><creator><name>Gavazzi G.</name></creator><creator><name>Franzetti P.</name></creator><creator><name>Scodeggio M.</name></creator><creator><name>Boselli A.</name></creator><date role="Updated">2024-06-27T20:18:11Z</date><date role="Created">2006-03-21T21:10:00Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>galaxies</subject><subject>surface-photometry</subject><subject>infrared-photometry</subject><subject>galaxy-classification-systems</subject><description>We present the distribution of a statistical sample of nearby galaxies in the {kappa}-space ({kappa1}{prop.to}logM, {kappa}2{prop.to}log(Ie)^3^*M/L, {kappa}3{prop.to}M/L). Our study is based on near-IR (H-band: {lamdba}=1.65{mu}m) observations, for the first time comprising early- and late-type systems. Our data confirm that the mean effective dynamical mass-to-light ratio M/L of the E+S0+S0a galaxies increases with increasing effective dynamical mass M, as expected from the existence of the Fundamental Plane relation. Conversely, spiral and Im/BCD galaxies show broad distribution in M/L with no detected trend of M/L with M, the former galaxies having M/L values about twice larger than the latter, on average. For all the late-type galaxies, the M/L increases with decreasing effective surface intensity Ie, consistent with the existence of the Tully-Fisher relation.</description><source format="bibcode">2002MNRAS.332..422P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/332/422</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/VII/49">VII/49 : Galaxies and Clusters of Galaxies (CGCG) (Zwicky, 1968)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/90/1681">J/AJ/90/1681 : The Virgo Cluster Catalog (VCC) (Binggeli+, 1985)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/120/489">J/A+AS/120/489 : Galaxies morphology and IR photometry I. (Gavazzi+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/142/65">J/A+AS/142/65 : Galaxies morphology and IR photometry III. (Gavazzi+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/142/73">J/A+AS/142/73 : Galaxies morphology and IR photometry IV. (Boselli+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/361/863">J/A+A/361/863 : Galaxies morphology and IR photometry V. 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