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<ri:Resource created="2015-03-04T06:46:32Z" 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>H{alpha} emission sources in h and {chi} Per</title><shortName>J/ApJ/669/L33</shortName><identifier>ivo://CDS.VizieR/J/ApJ/669/L33</identifier><altIdentifier>doi:10.26093/cds/vizier.16699033</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Currie T.</name></creator><creator><name>Kenyon S.J.</name></creator><creator><name>Balog Z.</name></creator><creator><name>Bragg A.</name></creator><creator><name>Tokarz S.</name></creator><date role="Updated">2015-03-04T05:48:10Z</date><date role="Created">2015-03-04T06:46:32Z</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>infrared-sources</subject><subject>accretion</subject><subject>infrared-photometry</subject><description>We report the discovery of accretion disks associated with ~13Myr old intermediate/low-mass stars in h and {chi} Persei. Optical spectroscopy of ~5000 stars in these clusters and a surrounding halo population reveal 32 A-K stars with Halpha emission. Matching these stars with 2MASS and optical photometry yields 25 stars with the highest probability of cluster membership and EW(Halpha)&gt;=5{AA}. 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