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<ri:Resource created="2016-03-24T08:42:42Z" 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>Molecular clouds and star formation</title><shortName>J/A+A/588/A104</shortName><identifier>ivo://CDS.VizieR/J/A+A/588/A104</identifier><altIdentifier>doi:10.26093/cds/vizier.35880104</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gong Y.</name></creator><creator><name>Mao R.Q.</name></creator><creator><name>Fang M.</name></creator><creator><name>Zhang S.B.</name></creator><creator><name>Su Y.</name></creator><creator><name>Yang J.</name></creator><creator><name>Jiang Z.B.</name></creator><creator><name>Xu Y.,Wang M.</name></creator><creator><name>Wang Y.</name></creator><creator><name>Lu D.R.</name></creator><creator><name>Sun J.X.</name></creator><date role="Updated">2018-05-11T15:16:39Z</date><date role="Created">2016-03-24T08:42:42Z</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>galaxy-planes</subject><subject>milky-way-galaxy</subject><subject>molecular-clouds</subject><subject>young-stellar-objects</subject><subject>co-line-emission</subject><description>As a part of the Milky Way Imaging Scroll Painting (MWISP) survey, the aim is to study the physical properties of molecular clouds and their associated star formation toward the Galactic plane within 216.25{deg}&lt;=l&lt;=218.75{deg} and -0.75{deg}&lt;=b&lt;=1.25{deg}, which covers the molecular cloud complex S287. 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