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<ri:Resource created="2005-09-14T21:55:16Z" 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>Substellar population of lambda Ori</title><shortName>J/ApJ/610/1064</shortName><identifier>ivo://CDS.VizieR/J/ApJ/610/1064</identifier><altIdentifier>doi:10.26093/cds/vizier.16101064</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Barrado Y Navascues D.</name></creator><creator><name>Stauffer J.R.</name></creator><creator><name>Bouvier J.</name></creator><creator><name>Jayawardhana R.,Cuillandre J.-C.</name></creator><date role="Updated">2005-09-14T21:57:42Z</date><date role="Created">2005-09-14T21:55:16Z</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>pre-main-sequence-stars</subject><subject>visible-astronomy</subject><subject>kron-cousins-photometry</subject><subject>infrared-photometry</subject><subject>spectroscopy</subject><description>By collecting optical and infrared photometry and low-resolution spectroscopy, we have identified a large number of low-mass stars and brown dwarf candidates belonging to the young cluster (~5Myr) associated with the binary star {lambda} Orionis. The lowest mass object found is an M8.5 with an estimated mass of 0.02M_{Sun}_ (~0.01M_{Sun}_ for objects without spectroscopic confirmation). For those objects with spectroscopy, the measured strength of the H{alpha} emission line follows a distribution similar to other clusters with the same age range, with larger equivalent widths for cooler spectral types.</description><source format="bibcode">2004ApJ...610.1064B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/610/1064</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/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/118/2409">J/AJ/118/2409 : {lambda} Ori PMS stars VRI photometry (Dolan+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/123/387">J/AJ/123/387 : {lambda} Ori star-forming region VRI photometry (Dolan+, 2002)</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/A+A/357/1001">J/A+A/357/1001 : {lambda}-Orionis ring in CO (Lang+ 2000)</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/610/1064</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/610/1064</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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