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<ri:Resource created="2023-09-14T15:25:18Z" status="active" updated="2025-06-13T15:25:00Z" 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>Velocity gradient and galaxy properties correlation</title><shortName>J/MNRAS/495/4820</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/495/4820</identifier><altIdentifier>doi:10.26093/cds/vizier.74954820</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lu S.</name></creator><creator><name>Cappellari M.</name></creator><creator><name>Mao S.</name></creator><creator><name>Ge J.</name></creator><creator><name>Li R.</name></creator><date role="Updated">2025-02-06T20:13:34Z</date><date role="Created">2023-09-14T15:25:18Z</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-radii</subject><subject>galaxy-kinematics</subject><subject>chemical-abundances</subject><subject>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>visible-astronomy</subject><description>Galaxy properties are known to correlate most tightly with the galaxy effective stellar velocity dispersion {sigma}_e_. Here, we look for additional trends at fixed {sigma}_e_ using 1339 galaxies (M_*_&gt;~6x10^9^M_{sun}_) with different morphologies in the MaNGA (DR14) sample with integral-field spectroscopy data. We focus on the gradients ({gamma}_rms_={sigma}(R_e_/4)/{sigma}_e_) of the stellar root-mean-square velocity (V_rms_=sqrt(V^2^+{sigma}^2^)), which we show traces the total mass density gradient {gamma}_tot_ derived from dynamical models and, more weakly, the bulge fraction. We confirm that {gamma}_rms_ increases with {sigma}_e_, age, and metallicity. We additionally find that these correlations still exist at fixed {sigma}_e_, where galaxies with larger {gamma}_rms_ are found to be older and more metal-rich. It means that mass density gradients contain information of the stellar population which is not fully accounted for by {sigma}_e_. This result puts an extra constraint on our understanding of galaxy quenching. We compare our results with galaxies in the IllustrisTNG hydrodynamical simulations and find that, at fixed {sigma}_e_, similar trends exist with age, the bulge fraction, and the total mass density slope but, unlike observations, no correlation with metallicity can be detected in the simulations.</description><source format="bibcode">2020MNRAS.495.4820L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/495/4820</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/AJ/154/86">J/AJ/154/86 : MaNGA catalog, DR15 (Wake+, 2017)</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/495/4820</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/495/4820</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/495/4820</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/495/4820</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/495/4820</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ID</name><description>MaNGA identifier (NN-NNNNNNNNN)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>logRe</name><description>Logarithm of the half-light radius R_e_</description><unit>log(arcsec)</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logRemaj</name><description>Logarithm of the major axis of the half-light isophote R_e_^maj^</description><unit>log(arcsec)</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logsigRe/4</name><description>Luminosity-weighted velocity dispersion within a circular aperture with radius R_e_/4 ({sigma}(R_e_/4))</description><unit>log(km.s**-1)</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logsigRe</name><description>Luminosity-weighted velocity dispersion within an elliptical aperture of area A={pi}R_e_^2^ ({sigma}_e_)</description><unit>log(km.s**-1)</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>gammarms</name><description>Gradient of the stellar root-mean-square velocity {gamma}_rms_={sigma}(R_e_/4)/{sigma}_e_</description><ucd>arith.grad;phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>gammatot</name><description>Mass-weighted total density slope from Li et al. 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