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<ri:Resource created="2013-03-26T12:07:11Z" status="active" updated="2025-06-13T15:25:00Z" 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>Properties of Collinder 69 low-mass members</title><shortName>J/A+A/547/A80</shortName><identifier>ivo://CDS.VizieR/J/A+A/547/A80</identifier><altIdentifier>doi:10.26093/cds/vizier.35470080</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bayo A.</name></creator><creator><name>Barrado D.</name></creator><creator><name>Huelamo N.</name></creator><creator><name>Morales-Calderon M.</name></creator><creator><name>Melo C.</name></creator><creator><name>Stauffer J.,Stelzer B.</name></creator><date role="Updated">2017-10-18T08:24:50Z</date><date role="Created">2013-03-26T12:07:11Z</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>early-type-stars</subject><subject>line-intensities</subject><description>Most observational studies conducted so far point toward brown dwarfs sharing a similar formation mechanism as the one that is accepted for low-mass stars. However, larger databases and more systematic studies are needed before strong conclusions can be reached. In this second paper of a series devoted to studying the spectroscopic properties of the Lambda Orionis star-forming region members, we study accretion, activity and rotation for a wide set of spectroscopically confirmed members of the central star cluster Collinder 69 to assess analogies and/or differences between the brown-dwarf and stellar populations of this cluster. Moreover, we present comparisons with other star-forming regions of similar and different ages to address environmental effects on our conclusions. We studied prominent photospheric lines to derive rotational velocities and emission lines to distinguish between accretion processes and chromospheric activity. In addition, we include information about disk presence and X-ray emission.</description><source format="bibcode">2012A&amp;A...547A..80B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/547/A80</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/AJ/118/2409">J/AJ/118/2409 : VRI photometry of lambda Ori PMS stars (Dolan+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/121/2124">J/AJ/121/2124 : lambda Ori pre-main-sequence stars photometry (Dolan+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/610/1064">J/ApJ/610/1064 : lambda Ori substellar population (Barrado y Navascues+ 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/664/481">J/ApJ/664/481 : Collinder 69 opt/IR photometry (Barrado y Navascues+ 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/488/167">J/A+A/488/167 : Low-mass stars in sigma Ori and lambda Ori (Sacco+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/492/277">J/A+A/492/277 : Analysis of Collinder 69 stars with VOSA (Bayo+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/385/2210">J/MNRAS/385/2210 : Spectroscopy around lam Ori and sig Ori (Maxted+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/526/A21">J/A+A/526/A21 : Collinder 69 X-ray sources (Barrado+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/536/A63">J/A+A/536/A63 : Collinder 69 very low mass stars &amp; brown dwarfs (Bayo+ 2011)</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/547/A80</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/547/A80</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/547/A80</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/547/A80</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/547/A80</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/547/A80</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/547/A80/table6 (Parameters and measurements obtained in this work for Collinder 69 confirmed members and comparison with previous studies)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/547/A80/table6?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/547/A80/table6?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/547/A80/table6?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>83.44658</ra><dec>9.92736</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/23717 23719 23728</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/547/A80?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/547/A80/table6</name><description>Parameters and measurements obtained in this work for Collinder 69 confirmed members and comparison with previous studies</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>e_W10(Ha)2</name><description>? 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