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<ri:Resource created="2018-10-23T09:52:13Z" status="active" updated="2025-06-13T15:25:00Z" 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>ALMA viewing of OH 231.8+4.2</title><shortName>J/A+A/618/A164</shortName><identifier>ivo://CDS.VizieR/J/A+A/618/A164</identifier><altIdentifier>doi:10.26093/cds/vizier.36180164</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sanchez Contreras C.</name></creator><creator><name>Alcolea J.</name></creator><creator><name>Bujarrabal V.</name></creator><creator><name>Castro-Carrizo A.,Velilla Prieto L.</name></creator><creator><name>Santander-Garcia M.</name></creator><creator><name>Quintana-Lacaci G.</name></creator><creator><name>Cernicharo J.</name></creator><date role="Updated">2018-11-05T10:52:51Z</date><date role="Created">2018-10-23T09:52:13Z</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>nebulae</subject><subject>molecular-clouds</subject><description>We present continuum and molecular line emission ALMA observations of OH 231.8+4.2, a well studied bipolar nebula around an asymptotic giant branch (AGB) star. The high angular resolution (~0.2"-0.3") and sensitivity of our ALMA maps provide the most detailed and accurate description of the overall nebular structure and kinematics of this object to date. We have identified a number of outflow components previously unknown. Species studied in this work include ^12^CO, ^13^CO, CS, SO, SO_2_, OCS, SiO, SiS, H_3_O^+^, Na^37^Cl, and CH_3_OH. 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