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<ri:Resource created="2010-03-26T13:59:52Z" 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>High mass protostellar objects physical parameters</title><shortName>J/A+A/498/147</shortName><identifier>ivo://CDS.VizieR/J/A+A/498/147</identifier><altIdentifier>doi:10.26093/cds/vizier.34980147</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Grave J.M.C.</name></creator><creator><name>Kumar M.S.N.</name></creator><date role="Updated">2017-12-07T07:27:34Z</date><date role="Created">2010-03-26T13:59:52Z</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>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><subject>galaxy-classification-systems</subject><description>In a previous work (Paper I, Kumar &amp; Grave, 2007A&amp;A...472..155K) a sample of 380 HMPO targets was studied using the GLIMPSE point source catalog and images. A colour-magnitude analysis of the point sources resulted in the identification of infrared counterparts (IRC) of the (sub)mm cores of HMPO candidates which were considered bona fide targets. 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