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<ri:Resource created="2011-10-14T15:27:14Z" 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>12mm line survey towards W28 SNR</title><shortName>J/MNRAS/411/1367</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/411/1367</identifier><altIdentifier>doi:10.26093/cds/vizier.74111367</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Nicholas B.</name></creator><creator><name>Rowell G.</name></creator><creator><name>Burton M.G.</name></creator><creator><name>Walsh A.</name></creator><creator><name>Fukui Y.</name></creator><creator><name>Kawamura A.,Longmore S.</name></creator><creator><name>Keto E.</name></creator><date role="Updated">2024-07-13T20:14:22Z</date><date role="Created">2011-10-14T15:27:14Z</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>supernovae</subject><subject>gamma-ray-astronomy</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><subject>radio-astronomy</subject><description>We present 12mm Mopra observations of dense molecular gas towards the W28 supernova remnant (SNR) field. The focus is on the dense molecular gas towards the TeV gamma-ray sources detected by the HESS telescopes, which likely trace the cosmic rays from W28 and possibly other sources in the region. 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