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<ri:Resource created="2025-02-13T14:52:20Z" status="active" updated="2025-07-18T20:17:16Z" 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>CRDs galaxies candidates in SDSS-IV MaNGA</title><shortName>J/MNRAS/511/139</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/511/139</identifier><altIdentifier>doi:10.26093/cds/vizier.75110139</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bevacqua D.</name></creator><creator><name>Cappellari M.</name></creator><creator><name>Pellegrini S.</name></creator><date role="Updated">2025-07-18T20:17:16Z</date><date role="Created">2025-02-13T14:52:20Z</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>galaxy-classification-systems</subject><subject>spectroscopy</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>stellar-masses</subject><subject>galaxy-radii</subject><subject>astrometry</subject><subject>stellar-ages</subject><subject>chemical-abundances</subject><subject>galaxy-kinematics</subject><description>We present the integral-field kinematics and stellar population properties of 64 galaxies (61 are Early-Type galaxies; ETGs) with Counter-Rotating stellar Disks (CRD) selected from about 4000 galaxies in the MaNGA survey, based on evidence of counter-rotation or two velocity dispersion peaks in the kinematic maps. For 17 CRDs, the counter-rotating components can also be separated spectroscopically. The frequency of CRDs in MaNGA is &lt;5 per cent for ellipticals, &lt;3 per cent for lenticulars, and &lt;1 per cent for spirals (at 95 per cent confidence level), consistent with previous estimates. We produced age and metallicity maps, and compared the stellar population properties to those of the general ETGs population. We found that CRDs have similar trends in age and metallicity to ETGs, but are less metallic at low masses, and show flatter age and steeper metallicity gradients, on average. A comparison of the velocity fields of the ionized gas and the stars reveals that in 33 cases the gas corotates with either the inner (15 cases) or outer (18 cases) stellar disc, and in nine cases it is misaligned. In most cases the gas corotates with the younger disc. Evidence of multimodality in the stellar population is found in 31 galaxies, while the 14 youngest and least massive galaxies show ongoing star formation; 14 galaxies, instead, exhibit unimodality, and are the oldest and most massive. As a general result, our work indicates that CRDs form primarily via gas accretion in retrograde rotation with respect to a pre-existing stellar disc.</description><source format="bibcode">2022MNRAS.511..139B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/511/139</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/MNRAS/477/4711">J/MNRAS/477/4711 : Stellar angular momentum for MaNGA galaxies (Graham+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/413/813">J/MNRAS/413/813 : ATLAS3D project. 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Difference of the kinematic position angles between the stellar and the gas velocity fields ({Delta}PA) (3)</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Pop</name><description>[young old nan] Correspond to the corotation of the gaseous disk with the younger or older disk (star/gas_vs.pop)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>logAge</name><description>Luminosity weighted mean age within 1 R_e_ as in the equation 8 of the section 4.1 Stellar population maps (log10&lt;Age&gt;)</description><unit>log(yr)</unit><ucd>phys.luminosity;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[M/H]</name><description>Luminosity weighted mean metallicity within 1 R_e_ as in the equation 9 of the section 4.1 Stellar population maps (&lt;[M/H]&gt;)</description><unit>log(Sun)</unit><ucd>phys.luminosity;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>GradAge</name><description>Gradient of Age (GradAge) (5)</description><unit>log(yr.kpc**-1)</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Grad[M/H]</name><description>Gradient of metallicity (Grad[M/H]) (5)</description><unit>log(Sun.kpc**-1)</unit><ucd>arith.grad;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Modality</name><description>Modality of the weights maps from regularized fits (Modality) (6)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>_RA</name><description>Positions from MaNGA catalog DR15 Cat. 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