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<ri:Resource created="2012-01-09T08:39:17Z" status="active" updated="2026-05-19T14:25:37Z" 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>Gas content of star-forming galaxies</title><shortName>J/ApJ/706/516</shortName><identifier>ivo://CDS.VizieR/J/ApJ/706/516</identifier><altIdentifier>doi:10.26093/cds/vizier.17060516</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pflamm-Altenburg J.</name></creator><creator><name>Kroupa P.</name></creator><date role="Updated">2026-05-19T14:25:37Z</date><date role="Created">2012-01-09T08:39:17Z</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>absolute-magnitude</subject><description>Stars do not form continuously distributed over star-forming galaxies. They form in star clusters of different masses. This nature of clustered star formation is taken into account in the theory of the integrated galactic stellar initial mass function (IGIMF) in which the galaxy-wide initial mass function (IMF) on galaxy-wide scales is calculated by adding all IMFs of young star clusters. For massive stars, the IGIMF is steeper than the universal IMF in star clusters and steepens with decreasing star formation rate (SFR) which is called the IGIMF effect. The current SFR and the total H{alpha} luminosity of galaxies therefore scale nonlinearly in the IGIMF theory compared to the classical case in which the galaxy-wide IMF is assumed to be constant and identical to the IMF in star clusters. Here we apply for the first time the revised SFR-L_H{alpha}_ relation on a sample of local volume star-forming galaxies with measured H{alpha} luminosities.</description><source format="bibcode">2009ApJ...706..516P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/706/516</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/III/167">III/167 : Atlas of UV spectra of star-forming galaxies (Kinney+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Ser/179.87">J/other/Ser/179.87 : H{alpha} in HII regions of Holmberg IX (Arbutina+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/476/1161">J/A+A/476/1161 : Spitzer photometry of M33 (Verley+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/164/81">J/ApJS/164/81 : Spectrophotometry of nearby galaxies (Moustakas+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/271">J/AJ/132/271 : SFR of M31 from resolved stars in near-IR (Olsen+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/338/525">J/MNRAS/338/525 : Recent star formation in UCM galaxies (Perez-Gonzalez+,</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/ApJ/706/516</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/706/516</mirrorURL><mirrorURL title="VizieR at SAAO: 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