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<ri:Resource created="2026-08-05T09:42:43Z" status="active" updated="2026-08-05T08:43:11Z" 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>Late-type gal. ultra-deep HI radial profiles</title><shortName>J/A+A/712/A74</shortName><identifier>ivo://CDS.VizieR/J/A+A/712/A74</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Veronese S.</name></creator><creator><name>de Blok W.J.G.</name></creator><creator><name>Brinks E.</name></creator><creator><name>Kleiner D.</name></creator><creator><name>Kurapati S.</name></creator><creator><name>Healy J.,Maccagni F.M.</name></creator><date role="Updated">2026-08-05T08:43:11Z</date><date role="Created">2026-08-05T09:42:43Z</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>radio-astronomy</subject><subject>h-i-line-emission</subject><description>Galaxy discs have a finite extent, yet how and where their neutral atomic hydrogen (HI) components end is not fully understood. The existence of a break in the HI disc at column densities of ~10^+19^cm^-2^ has been debated since early 21-cm observations of the spiral galaxy NGC 3198. We present the HI radial profiles of 16 star-forming, late-type galaxies from the MeerKAT HI Observations of Nearby Galactic Objects: Observing Southern Emitters (MHONGOOSE) survey spanning a range of HI mass from 10^+7^M_{sun}_ to 10^+10^M_{sun}_. We probed via spectral stacking their HI discs down to inclination-corrected column densities of a few times 10^+17^cm^-2^ at kpc resolution. The HI radial profiles of high-mass (MHI&gt;10^+9^M_{sun}_) galaxies are characterised by a inner plateau, followed by a knee at column densities of ~5x10^+20^cm^-2^, but no edges are unambiguously identified. The HI radial profiles of low-mass (MHI&lt;10^+9^M_{sun}-) galaxies shows a steeper decline and also no edges. We found that the profiles are self-similar when normalised to the radius at which a mass surface density of 0.01M_{sun}_/pc^2^ is reached, in agreement with recent literature results, but we also found a possible correlation between the normalisation radius and the environment, suggesting that environment contributes to the shaping of the HI distribution in galaxies. The emerging picture is that the diverse morphology of the HI radial profiles is difficult to interpret, and future studies with a larger sample are necessary for quantifying the contribution of internal and external processes acting at different levels for different galaxies.</description><source format="bibcode">2026A&amp;A...712A..74V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/712/A74</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/VIII/73">VIII/73 : HI Parkes All Sky Survey Catalogue (HIPASS) (Meyer+, 2004)</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/712/A74</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/712/A74</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/712/A74</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/712/A74</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/712/A74</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/712/A74</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/A+A/712/A74/table1 (Basic properties of the MHONGOOSE galaxies in our sample)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/712/A74/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/712/A74/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/712/A74/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>2.0556667</ra><dec>-34.5783333</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/16414 16441 16687 21026 24912 25077 25318 33920 33958 34476 34478 34501 35746 36131 43972 46491</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/712/A74?format=ascii</footprint><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/712/A74/table1</name><description>Basic properties of the MHONGOOSE galaxies in our sample</description><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HIPASS</name><description>HIPASS name (JHHMM+DD)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>Name</name><description>Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000.0)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000.0)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Dist</name><description>Distance</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(MHI)</name><description>HI mass</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>incl</name><description>Inclination angle (1)</description><unit>deg</unit><ucd>src.orbital.inclination</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>log(M*)</name><description>Stellar mass</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(SFR)</name><description>Star formation rate</description><unit>log(solMass.yr**-1)</unit><ucd>phys.SFR</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/712/A74/profiles</name><description>HI profiles of the 16 sources</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>HIPASS</name><description>HIPASS name (JHHMM+DD) (HIPASS)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>Raddeg</name><description>Galactocentric radius (radius_deg)</description><unit>deg</unit><ucd>phys.angSize;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Profs150-180</name><description>? Inclination-corrected radial profile from sector 150-180 deg (profile_s150_180)</description><unit>1e+19cm**-2</unit><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Profs180-210</name><description>? 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