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<ri:Resource created="2025-07-01T10:40:57Z" status="active" updated="2026-08-28T12:44:38Z" 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>Solar neighborhood clusters in moving-groups</title><shortName>J/A+A/699/L5</shortName><identifier>ivo://CDS.VizieR/J/A+A/699/L5</identifier><altIdentifier>doi:10.26093/cds/vizier/bc-nv/wf</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Swiggum C.</name></creator><creator><name>Alves J.</name></creator><creator><name>D'Onghia E.</name></creator><date role="Updated">2026-08-28T12:44:38Z</date><date role="Created">2025-07-01T10:40:57Z</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>open-star-clusters</subject><subject>stellar-associations</subject><description>Moving groups in the solar neighborhood are ensembles of co-moving stars, likely originating from spiral-arm resonances, the Galactic bar, or external perturbations. Their co-movement with young clusters indicates recent star formation, but a lack of precise 3-D positions and velocities has obscured the connection. Using backward-orbit integrations of 509 clusters within ~1kpc -- based on Gaia DR3 and supplemented with APOGEE-2 and GALAH DR3 radial velocities -- we trace their evolution over the past 100Myr. Most clusters separate into three spatial branches that trace the Pleiades, Coma Berenices, and Sirius moving groups; no analogous branch is seen for the Hyades group. Clusters belonging to the Alpha Persei, Messier 6, and Collinder 135 families, previously shown to have formed in three massive star-forming complexes, commove with either the Pleiades (Alpha Persei, Messier 6) or Coma Berenices (Collinder 135). Our results sharpen the view of how large-scale Galactic dynamics shape nearby star formation. The cluster sample is drawn from the young-cluster catalogue of Hunt &amp; Reffert (2023A&amp;A...673A.114H, Cat. J/A+A/673/A114).</description><source format="bibcode">2025A&amp;A...699L...5S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/699/L5</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/673/A114">J/A+A/673/A114 : Improving the open cluster census. II. (Hunt+, 2023)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/686/A42">J/A+A/686/A42 : Improving the open cluster census. III. 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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>Name</name><description>Cluster identifier (catalogue name)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>Age</name><description>Log-linear age estimate (Hunt &amp; Reffert, 2023, Cat. 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J/A+A/673/A114 (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>From Hunt et al., 2023, Cat. J/A+A/673/A114 (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>