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<ri:Resource created="2013-05-17T09:04:50Z" 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>Millimetric and far-IR maps of IRDC 18310-4</title><shortName>J/A+A/553/A115</shortName><identifier>ivo://CDS.VizieR/J/A+A/553/A115</identifier><altIdentifier>doi:10.26093/cds/vizier.35530115</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Beuther H.</name></creator><creator><name>Linz H.</name></creator><creator><name>Tackenberg J.</name></creator><creator><name>Henning Th.</name></creator><creator><name>Krause O.</name></creator><creator><name>Ragan S.,Nielbock M.</name></creator><creator><name>Launhardt R.</name></creator><creator><name>Bihr S.</name></creator><creator><name>Schmiedeke A.</name></creator><creator><name>Smith R.</name></creator><creator><name>Sakai T.</name></creator><date role="Updated">2022-12-19T07:36:48Z</date><date role="Created">2013-05-17T09:04:50Z</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>molecular-clouds</subject><subject>radio-spectroscopy</subject><description>Because of their short evolutionary time-scales, the earliest stages of high-mass star formation prior to the existence of any embedded heating source have barely been characterized until today. We study the fragmentation and dynamical properties of a massive starless gas clump at the onset of high-mass star formation. Based on Herschel continuum data we identify a massive gas clump that remains far-infrared dark up to 100um wavelengths. 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