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<ri:Resource created="2015-07-29T07:20:46Z" 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>SNR G18.8+0.3 data cubes</title><shortName>J/A+A/580/A51</shortName><identifier>ivo://CDS.VizieR/J/A+A/580/A51</identifier><altIdentifier>doi:10.26093/cds/vizier.35800051</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Paron S.</name></creator><creator><name>Celis Pena M.</name></creator><creator><name>Ortega M.E.</name></creator><creator><name>Petriella A.</name></creator><creator><name>Rubio M.</name></creator><creator><name>Dubner G.,Giacani E.</name></creator><date role="Updated">2015-12-02T07:28:18Z</date><date role="Created">2015-07-29T07:20:46Z</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>supernova-remnants</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><description>In a previous paper we investigated the molecular environment toward the eastern border of the supernova remnant (SNR) G18.8+0.3. Continuing with the study of the surroundings of this SNR, we now focus on its southern border, which in the radio continuum emission shows a very peculiar morphology with a corrugated corner and a very flattened southern flank. We observed two regions toward the south of SNR G18.8+0.3 using the Atacama Submillimeter Telescope Experiment (ASTE) in the ^12^CO J=3-2. One of these regions was also surveyed in ^13^ CO and C^18^O J=3-2. The angular and spectral resolution of these observations were 22" and 0.11km/s. 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