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<ri:Resource created="2008-08-16T05:42:38Z" 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>Age-metallicity relation of {omega} Cen</title><shortName>J/ApJ/647/1075</shortName><identifier>ivo://CDS.VizieR/J/ApJ/647/1075</identifier><altIdentifier>doi:10.26093/cds/vizier.16471075</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Stanford L.M.</name></creator><creator><name>Da Costa G.S.</name></creator><creator><name>Norris J.E.</name></creator><creator><name>Cannon R.D.</name></creator><date role="Updated">2008-08-16T05:45:40Z</date><date role="Created">2008-08-16T05:42:38Z</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>globular-star-clusters</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>radial-velocity</subject><subject>metallicity</subject><description>We present a metallicity distribution based on photometry and spectra for 442 Omega Centauri cluster members that lie at the main-sequence turnoff region of the color-magnitude diagram. This distribution is similar to that found for the red giant branch. The distribution shows a sharp rise to a mean of [Fe/H]=-1.7 with a long tail to higher metallicities. Ages have then been determined for the stars using theoretical isochrones enabling the construction of an age-metallicity diagram. Interpretation of this diagram is complicated by the correlation of the errors in the metallicities and ages. Nevertheless, after extensive Monte Carlo simulations, we conclude that our data show that the formation of the cluster took place over an extended period of time: the most metal-rich stars in our sample ([Fe/H]~-0.6) are younger by 2-4Gyr than the most metal-poor population.</description><source format="bibcode">2006ApJ...647.1075S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/647/1075</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/250/314">J/MNRAS/250/314 : CCD photometry of omega Cen (Noble+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/106/828">J/PASP/106/828 : BVRI photometry of Omega Cen (Walker 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/114/1087">J/AJ/114/1087 : Omega Cen radial velocities (Mayor+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/958">J/AJ/127/958 : CCD BV photometry on Omega Cen (Rey+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/445/503">J/A+A/445/503 : Radial velocities in Omega Cen (NGC5139) (Reijns+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/1395">J/AJ/135/1395 : omega Cen Spitzer photometry (Boyer+, 2008)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/647/1075</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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