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<ri:Resource created="2013-10-28T09:26:10Z" 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>The Red MSX Source Survey: massive protostars</title><shortName>J/ApJS/208/11</shortName><identifier>ivo://CDS.VizieR/J/ApJS/208/11</identifier><altIdentifier>doi:10.26093/cds/vizier.22080011</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lumsden S.L.</name></creator><creator><name>Hoare M.G.</name></creator><creator><name>Urquhart J.S.</name></creator><creator><name>Oudmaijer R.D.</name></creator><creator><name>Davies B.,Mottram J.C.</name></creator><creator><name>Cooper H.D.B.</name></creator><creator><name>Moore T.J.T.</name></creator><date role="Updated">2017-09-22T16:16:08Z</date><date role="Created">2013-10-28T09:26:10Z</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>infrared-sources</subject><subject>stellar-distance</subject><subject>surveys</subject><subject>h-ii-regions</subject><subject>young-stellar-objects</subject><subject>late-type-stars</subject><description>We present the Red MSX Source survey, the largest statistically selected catalog of young massive protostars and H II regions to date. We outline the construction of the catalog using mid- and near-infrared color selection. We also discuss the detailed follow up work at other wavelengths, including higher spatial resolution data in the infrared. We show that within the adopted selection bounds we are more than 90% complete for the massive protostellar population, with a positional accuracy of the exciting source of better than 2 arcsec. We briefly summarize some of the results that can be obtained from studying the properties of the objects in the catalog as a whole; we find evidence that the most massive stars form: (1) preferentially nearer the Galactic center than the anti-center; (2) in the most heavily reddened environments, suggestive of high accretion rates; and (3) from the most massive cloud cores.</description><source format="bibcode">2013ApJS..208...11L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/208/11</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/V/114">V/114 : MSX6C infrared point source catalog (Egan+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/410/1237">J/MNRAS/410/1237 : Red MSX survey (RMS) massive young stars (Urquhart+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/418/1689">J/MNRAS/418/1689 : Red MSX water maser and ammonia emissions (Urquhart+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/525/A149">J/A+A/525/A149 : RMS: bolometric fluxes of YSOs (Mottram+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/94">J/AJ/142/94 : Red MSX sources in BGPS (Schenck+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/507/795">J/A+A/507/795 : The RMS survey: water masers of YSOs (Urquhart+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/122/1844">J/AJ/122/1844 : MSX and 2MASS cross-correlation in LMC (Egan+, 2001)</relatedResource><relatedResource>http://rms.leeds.ac.uk/ : Online definitive version 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