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<ri:Resource created="2012-09-27T09:26:23Z" 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>22-GHz water maser clouds</title><shortName>J/A+A/546/A16</shortName><identifier>ivo://CDS.VizieR/J/A+A/546/A16</identifier><altIdentifier>doi:10.26093/cds/vizier.35460016</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Richards A.M.S.</name></creator><creator><name>Etoka S.</name></creator><creator><name>Gray M.D.</name></creator><creator><name>Lekht E.E.</name></creator><creator><name>Mendoza-Torres J.E.,Murakawa K.</name></creator><creator><name>Rudnitskij G.</name></creator><creator><name>Yates J.A.</name></creator><date role="Updated">2022-05-11T08:54:42Z</date><date role="Created">2012-09-27T09:26:23Z</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>supergiant-stars</subject><subject>astrophysical-masers</subject><subject>radio-astronomy</subject><description>Cool, evolved stars undergo copious mass loss but the detailed mechanisms and the form in which the matter is returned the ISM are still under debate. 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