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<ri:Resource created="2008-04-15T10:27:33Z" 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>Low-mass stars in the Cepheus OB2 region</title><shortName>J/AJ/128/805</shortName><identifier>ivo://CDS.VizieR/J/AJ/128/805</identifier><altIdentifier>doi:10.26093/cds/vizier.51280805</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sicilia-Aguilar A.</name></creator><creator><name>Hartmann L.W.</name></creator><creator><name>Briceno C.</name></creator><creator><name>Muzerolle J.</name></creator><creator><name>Calvet N.</name></creator><date role="Updated">2008-04-15T10:29:10Z</date><date role="Created">2008-04-15T10:27:33Z</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>stellar-spectral-types</subject><subject>line-intensities</subject><subject>visible-astronomy</subject><subject>kron-cousins-photometry</subject><subject>infrared-photometry</subject><subject>pre-main-sequence-stars</subject><description>We present the first identification of low-mass (spectral types K-M) stars in the young clusters Tr37 and NGC7160, members of the CepOB2 association. This is part of a program to follow the evolution of protoplanetary accretion disks through the ages thought to be crucial to understanding disk dissipation and planet formation (~3-10Myr). 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