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<ri:Resource created="2026-03-16T10:38:21Z" status="active" updated="2026-03-16T09:39:22Z" 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 galaxies morpho-kinematic class</title><shortName>J/A+A/707/A302</shortName><identifier>ivo://CDS.VizieR/J/A+A/707/A302</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pacheco-Arias J.</name></creator><creator><name>Amram P.</name></creator><creator><name>Epinat B.</name></creator><creator><name>Mercier W.</name></creator><date role="Updated">2026-03-16T09:39:22Z</date><date role="Created">2026-03-16T10:38:21Z</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>galaxy-classification-systems</subject><subject>visible-astronomy</subject><description>The two-dimensional spatial distribution of stellar specific angular momentum (sAM) within galaxies has never been analyzed to date. We seek to identify the morpho-kinematics of this property and its correlation with the total stellar sAM (j*) and the total stellar mass (M*) of late-type galaxies in the local universe. We estimate the two-dimensional distribution of stellar sAM for 30 spiral and irregular galaxies, mostly located in nearby low-density environments, part of the Gassendi H{alpha} survey of SPirals (GHASP). To do so, we produce for the first time, high-resolution stellar sAM surface density (sAMSD) maps by using a formalism which combines the 3.4um WISE photometry with H{alpha} velocity fields and rotation curves. The features of these new maps are quantified using standard non-parametric morphological indicators such as concentration, asymmetry, and smoothness, augmented by two additional coefficients that respectively measure the degree of similarity to an axisymmetric Freeman disc and the prominence of bi-symmetric substructures within the stellar sAMSD space. Each galaxy in our sample is classified into one of the five new morpho-kinematic categories proposed in this study: j*- ring, j*- spiral, j*- bar, j*- clump and j*- irregular. These classes are named after the predominant galactic substructure of their stellar sAMSD map and form a new classification scheme that combines both morphological characteristics and dynamic properties. For 14 galaxies, the morphological classification does not coincide with the corresponding morpho-kinematic category. As expected, there is a high correlation between j* and M* for our sample. Similarly, our galaxies exhibit a correlation between j* and their star formation rate, and between j* and their total mass. The mean j* and M* are distributed along different regions along the Fall relation for all j*- types, although there is a considerable scatter within each type. There is a link between the two-dimensional distribution of stellar sAMSD and j*. The location of the different j*- types in the j*-M* diagram could indicate a morpho-kinematic evolution of late-type galaxies within the hierarchical paradigm of galaxy formation. The physical mechanisms capable of modifying the shape of galaxies in the stellar sAMSD space seem to be related with the stability of the galactic disc. The spatial redistribution of angular momentum for low-mass late-type galaxies may be driven by a combination of feedback, dynamical friction, shock waves and resonances, while the quasi-stationary rotating density wave can be responsible for the aforementioned process in the massive spirals.</description><source format="bibcode">2026A&amp;A...707A.302P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/707/A302</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></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/707/A302</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/707/A302</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/707/A302</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/707/A302</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/707/A302</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/707/A302</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/707/A302/tablea1 (Galaxy parameters)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/707/A302/tablea1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/707/A302/tablea1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/707/A302/tablea1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>36.8196</ra><dec>33.579</dec><sr>0.005555555555555556</sr></testQuery></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/A+A/707/A302/list (List of fits maps)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/707/A302/list?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/707/A302/list?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/707/A302/list?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>236.37091</ra><dec>62.31375</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/2311 2320 3516 3860 5581 5596 5639 5710 6619 6623 6948 7110 7303 7957 9869 10841-10842 10935 10976 11127 11389 11443 11448 11566 11582 11639 11649 12047 12122 13162 13472 13489-13490 15592-15593 20270 28155 28496</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/707/A302?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/707/A302/table1</name><description>*Average parameters by morpho-kinematic category</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>Class</name><description>Morpho-kinematic category</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>Ngal</name><description>Number of galaxies in each category</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ttype</name><description>Mean morphological type code</description><ucd>meta.code;src.morph.type</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Ttype</name><description>1-sigma standard deviation of Ttype</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMstar</name><description>Mean stellar mass (log10)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logMstar</name><description>1-sigma standard deviation of logMstar</description><unit>log(solMass)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logjstar</name><description>Mean stellar specific angular momentum (log10)</description><unit>log(kpc.km.s**-1)</unit><ucd>phys.angMomentum;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logjstar</name><description>1-sigma standard deviation of logjstar</description><unit>log(kpc.km.s**-1)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R2</name><description>Mean ringness parameter</description><ucd>src.morph.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_R2</name><description>1-sigma standard deviation of R2</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>A2</name><description>Mean bar predominance parameter</description><ucd>src.morph.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_A2</name><description>1-sigma standard deviation of A2</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>C</name><description>Mean concentration index</description><ucd>meta.code;spect.index;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_C</name><description>1-sigma standard deviation of C</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>A</name><description>Mean asymmetry index</description><ucd>meta.code;spect.index;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_A</name><description>1-sigma standard deviation of A</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S</name><description>Mean smoothness index</description><ucd>src.morph.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_S</name><description>1-sigma standard deviation of S</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/A+A/707/A302/tablea1</name><description>Galaxy parameters</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. 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