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<ri:Resource created="2000-06-03T10:33:22Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Photometry of young star groupings in spirals</title><shortName>J/A+A/357/437</shortName><identifier>ivo://CDS.VizieR/J/A+A/357/437</identifier><altIdentifier>doi:10.26093/cds/vizier.33570437</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Battinelli P.</name></creator><creator><name>Capuzzo-Dolcetta R.</name></creator><creator><name>Hodge P.W.</name></creator><creator><name>Vicari A.</name></creator><creator><name>Wyder T.K.</name></creator><date role="Updated">2000-06-03T10:33:28Z</date><date role="Created">2000-06-03T10:33:22Z</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>photometry</subject><subject>stellar-populations</subject><subject>young-stellar-objects</subject><description>We present multiband photometric observations of three spiral galaxies selected in a sample suited for the study of young stellar groupings and their relationship with the parent galaxy and the galactic environment. Star forming regions have been identified using an objective technique based on a multivariate statistical analysis. Maps of young star groupings are given for each galaxy. The luminosity functions of the young star group populations show a remarkable similarity with a slope in the range -1.52 to -1.33. The size distributions peak around the classical 100pc value of the Local Group associations for two out of the three galaxies. NGC 1058 shows smaller associations (peak at ~50pc). The total number of young groups per unit B absolute luminosity of the galaxy is significantly greater in UGC 12732. The activity of star formation is in all three galaxies clearly stronger in the central regions.</description><source format="bibcode">2000A&amp;A...357..437B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/357/437</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/116/1626">J/AJ/116/1626 : Spiral &amp; lenticular galaxy brightness profiles (Baggett+, 1998</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/309/749">J/A+A/309/749 : Fundamental plane of early type galaxies (Prugniel+ 1996)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/357/437</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/357/437</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/357/437</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/357/437</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/357/437</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/357/437</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/357/437/table1</name><description>Young star groupings in NGC 7217</description><column><name>Seq</name><description>Identification number</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>X</name><description>Offset from the galactic centre (1)</description><unit>arcsec</unit><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Y</name><description>Offset from the galactic centre (1)</description><unit>arcsec</unit><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Dist</name><description>Distance to the centre</description><unit>kpc</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Bmag</name><description>? Integrated B magnitude (2)</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SuBr</name><description>? B-surface brightness (2)</description><unit>mag.arcsec**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>D</name><description>Size</description><unit>pc</unit><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/A+A/357/437/table2</name><description>Young star groupings in NGC 1058</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Seq</name><description>Identification number</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>X</name><description>Offset from the galactic centre (1)</description><unit>arcsec</unit><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Y</name><description>Offset from the galactic centre (1)</description><unit>arcsec</unit><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Dist</name><description>Distance to the centre</description><unit>kpc</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Bmag</name><description>? Integrated B magnitude (2)</description><unit>mag</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SuBr</name><description>? B-surface brightness (2)</description><unit>mag.arcsec**-2</unit><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>D</name><description>Size</description><unit>pc</unit><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/A+A/357/437/table3</name><description>Young star groupings in UGC 12732</description><column><name>Seq</name><description>Identification number</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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