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<ri:Resource created="2002-06-08T20:15:50Z" 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>Galactic orbits of stars with planets</title><shortName>J/A+A/384/879</shortName><identifier>ivo://CDS.VizieR/J/A+A/384/879</identifier><altIdentifier>doi:10.26093/cds/vizier.33840879</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Barbieri M.</name></creator><creator><name>Gratton R.G.</name></creator><date role="Updated">2019-04-08T13:41:53Z</date><date role="Created">2002-06-08T20:15:50Z</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>stellar-ages</subject><subject>stellar-masses</subject><subject>radial-velocity</subject><subject>proper-motions</subject><subject>metallicity</subject><description>We have reconstructed the galactic orbits of the parent stars of exoplanets. For comparison, we have recalculated the galactic orbits of stars from the Edvardsson et al. (1993, Cat. &lt;J/A+A/275/101&gt;) catalog. A comparison between the two samples indicates that stars with planets are not kinematically peculiar. At each perigalactic distance stars with planets have a metallicity systematically larger than the average for the comparison sample. We argue that this result favors scenarios where the presence of planets is the cause of the higher metallicity of stars with planets.</description><source format="bibcode">2002A&amp;A...384..879B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/384/879</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/275/101">J/A+A/275/101 : Chemical evolution of the galactic disk I. 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Age error</description><unit>Gyr</unit><ucd>stat.error;time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Mass</name><description>Mass</description><unit>Sun</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mass</name><description>? Mass error</description><unit>Sun</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/A+A/384/879/table4</name><description>Orbital data of stars with planets (SWP)</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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