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<ri:Resource created="2015-11-23T07:41:51Z" 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>IRDC18223 images</title><shortName>J/A+A/584/A67</shortName><identifier>ivo://CDS.VizieR/J/A+A/584/A67</identifier><altIdentifier>doi:10.26093/cds/vizier.35840067</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Beuther H.</name></creator><creator><name>Ragan S.E.</name></creator><creator><name>Johnston K.</name></creator><creator><name>Henning T.</name></creator><creator><name>Hacar A.</name></creator><creator><name>Kainulainen J.T.</name></creator><date role="Updated">2015-12-02T07:31:08Z</date><date role="Created">2015-11-23T07:41:51Z</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>early-type-stars</subject><subject>molecular-clouds</subject><description>Filamentary structures in the interstellar medium are crucial ingredients of the star formation process. They fragment to form individual star-forming cores, and at the same time they may also funnel gas toward the central gas cores, providing an additional gas reservoir. We want to resolve the length scales for filament formation and fragmentation (resolution &lt;=0.1pc), in particular the Jeans length and cylinder fragmentation scale. 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