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<ri:Resource created="2023-10-09T10:32:33Z" 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>Low-rotating elliptical galaxies in MaNGA</title><shortName>J/ApJ/863/107</shortName><identifier>ivo://CDS.VizieR/J/ApJ/863/107</identifier><altIdentifier>doi:10.26093/cds/vizier.18630107</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Durazo R.</name></creator><creator><name>Hernandez X.</name></creator><creator><name>Cervantes Sodi B.</name></creator><creator><name>Sanchez S.F.</name></creator><date role="Updated">2023-12-14T01:17:02Z</date><date role="Created">2023-10-09T10:32:33Z</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>galaxy-radii</subject><subject>galaxy-kinematics</subject><description>Pressure-supported systems modeled under Modified Newtonian dynamics (MOND)ian extended gravity are expected to show an outer flattening in their velocity dispersion profiles. A characteristic scaling between the amplitude of the asymptotic velocity dispersion and the radius at which the flattening occurs is also expected. By comprehensively analyzing the dynamical behavior of ~300 extremely low-rotating elliptical galaxies from the Mapping Nearby Galaxies at APO (MaNGA) survey, we show this type of pressure-supported system to be consistent with MONDian expectations, for a range of central velocity dispersion values of 60 km s^-1^&lt;{sigma}_central_&lt;280km/s and asymptotic velocity dispersion values of 28km/s&lt;{sigma}_\infty_&lt;250km/s. We find that a universal velocity dispersion profile accurately describes the studied systems; the predicted kinematics of extended gravity are verified for all well-observed galaxies.</description><source format="bibcode">2018ApJ...863..107D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/863/107</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/462/L9">J/A+A/462/L9 : Radial velocities in NGC 7099 (Scarpa+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/525/A148">J/A+A/525/A148 : Radial velocities in two globular clusters (Scarpa+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/530/A31">J/A+A/530/A31 : Stellar parameters in 10 globular cluster fields (Lane+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/738/186">J/ApJ/738/186 : HST and DEIMOS measurements of NGC 2419 stars (Ibata+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/544/A115">J/A+A/544/A115 : Velocities of NGC 4636 globular clusters (Schuberth+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/560/A9">J/A+A/560/A9 : AMIGA. 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