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<ri:Resource created="2017-11-27T12:35:19Z" 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>HI size-mass relation of galaxies</title><shortName>J/MNRAS/460/2143</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/460/2143</identifier><altIdentifier>doi:10.26093/cds/vizier.74602143</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wang J.</name></creator><creator><name>Koribalski B.S.</name></creator><creator><name>Serra P.</name></creator><creator><name>van der Hulst T.</name></creator><creator><name>Roychowdhury S.,Kamphuis P.</name></creator><creator><name>Chengalur J.N.</name></creator><date role="Updated">2024-08-16T20:17:15Z</date><date role="Created">2017-11-27T12:35:19Z</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>catalogs</subject><subject>h-i-line-emission</subject><subject>galaxy-classification-systems</subject><description>We revisit the HI size-mass (D_HII_-M_HI_) relation of galaxies with a sample of more than 500 nearby galaxies covering over five orders of magnitude in HI mass and more than 10 B-band magnitudes. The relation is remarkably tight with a scatter {sigma}~0.06dex, or 14 per cent. The scatter does not change as a function of galaxy luminosity, HI richness or morphological type. The relation is linked to the fact that dwarf and spiral galaxies have a homogeneous radial profile of HI surface density in the outer regions when the radius is normalized by D_HI_. The early-type disc galaxies typically have shallower HI radial profiles, indicating a different gas accretion history. We argue that the process of atomic-to-molecular gas conversion or star formation cannot explain the tightness of the D_HI_-M_HI_ relation. This simple relation puts strong constraints on simulation models for galaxy formation.</description><source format="bibcode">2016MNRAS.460.2143W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/460/2143</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/J/A+A/324/877">J/A+A/324/877 : HI properties of spiral and irregular galaxies (Broeils+, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/442/137">J/A+A/442/137 : HI observations of WHISP disk galaxies (Noordermeer+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/16">J/AJ/144/16 : Optical and HI properties of galaxies in voids (Kreckel+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/370/765">J/A+A/370/765 : HI synthesis observations in UMa cluster (Verheijen+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/2563">J/AJ/136/2563 : HI Nearby Galaxy Survey, THINGS (Walter+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/134">J/AJ/144/134 : LITTLE THINGS survey of nearby dwarf galaxies (Hunter+, 2012)</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/MNRAS/460/2143</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/460/2143</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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