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<ri:Resource created="2009-05-30T16:37:44Z" 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>JHKs and GLIMPSE photometry of RCW 120</title><shortName>J/A+A/496/177</shortName><identifier>ivo://CDS.VizieR/J/A+A/496/177</identifier><altIdentifier>doi:10.26093/cds/vizier.34960177</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Deharveng</name></creator><creator><name>L.</name></creator><creator><name>Zavagno A.</name></creator><creator><name>Schuller F.</name></creator><creator><name>Caplan J.</name></creator><creator><name>Pomares M.</name></creator><creator><name>De Breuck C.</name></creator><date role="Updated">2009-05-30T16:43:15Z</date><date role="Created">2009-05-30T16:37:44Z</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>h-ii-regions</subject><subject>early-type-stars</subject><subject>infrared-photometry</subject><description>This study deals with the star formation triggered by HII regions. We wish to take advantage of the very simple morphology of RCW 120 - a perfect bubble - to understand the mechanisms triggering star formation around an HII region and to establish what kind of stars are formed there. We present 870um observations of RCW 120, obtained with the APEX-LABOCA camera. These show the distribution of cold dust, and thus of neutral material. 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