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<ri:Resource created="2011-09-13T08:21:49Z" 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>Missing low-mass stars in S254-S258</title><shortName>J/A+A/533/A121</shortName><identifier>ivo://CDS.VizieR/J/A+A/533/A121</identifier><altIdentifier>doi:10.26093/cds/vizier.35330121</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mucciarelli P.</name></creator><creator><name>Preibisch T.</name></creator><creator><name>Zinnecker H.</name></creator><date role="Updated">2017-07-06T06:25:33Z</date><date role="Created">2011-09-13T08:21:49Z</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>pre-main-sequence-stars</subject><subject>young-stellar-objects</subject><subject>protostars</subject><subject>x-ray-sources</subject><description>The aim of this study was to find an explanation for the remarkable morphology of the central part of the S254-S258 star forming complex. We performed a deep Chandra X-ray observation of the S254-S258 region in order to efficiently discriminate young stars (with and without circumstellar matter) from the numerous older field stars in the area. We detected 364 X-ray point sources in a 17'x17' field. 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