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<ri:Resource created="2009-12-09T22:05:04Z" 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>Equivalent widths of IC 2602 &amp; IC 2391 stars</title><shortName>J/A+A/501/553</shortName><identifier>ivo://CDS.VizieR/J/A+A/501/553</identifier><altIdentifier>doi:10.26093/cds/vizier.35010553</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>D'Orazi V.</name></creator><creator><name>Randich S.</name></creator><date role="Updated">2009-12-09T21:12:31Z</date><date role="Created">2009-12-09T22:05:04Z</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>chemical-abundances</subject><description>Galactic open clusters have been long recognized as one of the best tools to investigate the chemical content of Galactic disk and its time evolution. In the last decade, many efforts have been directed to chemically characterize the old and intermediate age population; surprisingly, the chemical content of the younger and close counterpart remains largely undetermined. In this paper we present the abundance analysis of a sample of 15 G/K members of the young pre-main sequence clusters IC 2602 and IC 2391. Along with IC 4665, these are the first pre-main sequence clusters for which a detailed abundance determination has been carried out so far.</description><source format="bibcode">2009A&amp;A...501..553D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/501/553</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+AS/126/81">J/A+AS/126/81 : IC 2602 VRI photometry (Foster+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/126/357">J/A+AS/126/357 : Members of IC 2391 (Rolleston+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/372/862">J/A+A/372/862 : Lithium abundances in IC 2602 and IC 2391 (Randich+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/134/103">J/ApJS/134/103 : Low-mass members of IC 2391 (Barrado y Navascues+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/355/959">J/MNRAS/355/959 : Proper motions of IC 2391 possible members (Dodd+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/430/287">J/A+A/430/287 : XMM observations of IC 2391 stars (Marino+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/461/509">J/A+A/461/509 : Membership and spectroscopy of IC 2391 (Platais+, 2007)</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/A+A/501/553</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/501/553</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/501/553</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/501/553</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/501/553</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/501/553</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/A+A/501/553/stars (Sample stars)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/501/553/stars?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/501/553/stars?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/501/553/stars?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>157.130417</ra><dec>-63.7375</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/37229-37231 37240 37316 37318 37787-37788 37790</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/501/553?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/501/553/stars</name><description>Sample stars</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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