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<ri:Resource created="2008-03-30T17:00:36Z" 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>Fundamental parameters of five old open clusters</title><shortName>J/A+A/476/217</shortName><identifier>ivo://CDS.VizieR/J/A+A/476/217</identifier><altIdentifier>doi:10.26093/cds/vizier.34760217</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Carraro G.</name></creator><creator><name>Geisler D.</name></creator><creator><name>Villanova S.</name></creator><creator><name>Frinchaboy P.M.</name></creator><creator><name>Majewski S.R.</name></creator><date role="Updated">2019-05-08T15:16:15Z</date><date role="Created">2008-03-30T17:00:36Z</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>radial-velocity</subject><subject>metallicity</subject><subject>photometry</subject><description>The outer parts of the Milky Way disk are believed to be one of the main arenas where the accretion of external material in the form of dwarf galaxies and subsequent formation of streams is taking place. The Monoceros stream and the Canis Major and Argo over-densities are notorious examples. Understanding whether what we detect is the signature of accretion or, more conservatively, simply the intrinsic nature of the disk, represents one of the major goals of modern Galactic astronomy. We try to shed more light on the properties of the outer disk by exploring the properties of distant anti-center old open clusters. We want to verify whether distant clusters follow the chemical and dynamical behavior of the solar vicinity disk, or whether their properties can be better explained in terms of an extra-galactic population.</description><source format="bibcode">2007A&amp;A...476..217C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/476/217</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/442/917">J/A+A/442/917 : BVI photometry in Berkeley 73, 75 and 25 (Carraro+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/360/655">J/MNRAS/360/655 : 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