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<ri:Resource created="2007-03-12T13:13:54Z" 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>H{alpha} scale length in Virgo and field spirals</title><shortName>J/AJ/131/716</shortName><identifier>ivo://CDS.VizieR/J/AJ/131/716</identifier><altIdentifier>doi:10.26093/cds/vizier.51310716</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Koopmann R.A.</name></creator><creator><name>Haynes M.P.</name></creator><creator><name>Catinella B.</name></creator><date role="Updated">2017-09-27T05:55:29Z</date><date role="Created">2007-03-12T13:13:54Z</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>galaxy-clusters</subject><subject>galaxy-classification-systems</subject><description>The scale lengths of the old stars and ionized gas distributions are compared for similar samples of Virgo Cluster members and field spiral galaxies via H{alpha} and broad R-band surface photometry. While the R-band and H{alpha} scale lengths are, on average, comparable for the combined sample, we find significant differences between the field and cluster samples. While the H{alpha} scale lengths of the field galaxies are a factor of 1.14+/-0.07 longer, on average, than their R-band scale lengths, the H{alpha} scale lengths of Virgo Cluster members are, on average, 20% smaller than their R-band scale lengths.</description><source format="bibcode">2006AJ....131..716K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/131/716</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/26">VII/26 : Uppsala General Catalogue of Galaxies (UGC) (Nilson 1973)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/34">VII/34 : ESO/Uppsala Survey of the ESO(B) Atlas (Lauberts 1982)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/51">VII/51 : Revised Shapley-Ames Catalog of Bright Galaxies (Sandage+ 1981)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/62">VII/62 : Morphological Cat. of Gal. 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