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<ri:Resource created="2014-10-15T08:47:19Z" 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>APEX spectra of massive YSOs</title><shortName>J/A+A/570/A49</shortName><identifier>ivo://CDS.VizieR/J/A+A/570/A49</identifier><altIdentifier>doi:10.26093/cds/vizier.35700049</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Leurini S.</name></creator><creator><name>Codella C.</name></creator><creator><name>Lopez-Sepulcre A.</name></creator><creator><name>Gusdorf A.</name></creator><creator><name>Csengeri T.,Anderl S.</name></creator><date role="Updated">2018-05-01T14:21:49Z</date><date role="Created">2014-10-15T08:47:19Z</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>young-stellar-objects</subject><subject>spectroscopy</subject><description>Molecular outflows are a direct consequence of accretion, and therefore they represent one of the best tracers of accretion processes in the still poorly understood early phases of high-mass star formation. Previous studies suggested that the SiO abundance decreases with the evolution of a massive young stellar object probably because of a decay of jet activity, as witnessed in low-mass star-forming regions. 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