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<ri:Resource created="2017-03-17T07:43:58Z" 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>M 2-9 ^12^CO and ^13^CO channel maps</title><shortName>J/A+A/600/A4</shortName><identifier>ivo://CDS.VizieR/J/A+A/600/A4</identifier><altIdentifier>doi:10.26093/cds/vizier.36000004</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Castro-Carrizo A.</name></creator><creator><name>Bujarrabal V.</name></creator><creator><name>Neri R.</name></creator><creator><name>Alcolea J.,Sanchez Contreras C.</name></creator><creator><name>Santander-Garcia M.</name></creator><creator><name>Nyman L.-A.</name></creator><date role="Updated">2017-05-22T15:02:45Z</date><date role="Created">2017-03-17T07:43:58Z</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>planetary-nebulae</subject><subject>radial-velocity</subject><subject>radio-astronomy</subject><description>M 2-9 is a young planetary nebula (PN) that shows the characteristics of its last ejections in unprecedented detail. These last ejections are thought to trigger the post-asymptotic giant branch evolution. 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