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<ri:Resource created="2011-05-16T14:49:40Z" 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>Dense cores in Perseus</title><shortName>J/ApJ/696/298</shortName><identifier>ivo://CDS.VizieR/J/ApJ/696/298</identifier><altIdentifier>doi:10.26093/cds/vizier.16960298</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Foster J.B.</name></creator><creator><name>Rosolowsky E.W.</name></creator><creator><name>Kauffmann J.</name></creator><creator><name>Pineda J.E.</name></creator><creator><name>Borkin M.A.,Caselli P.</name></creator><creator><name>Myers P.C.</name></creator><creator><name>Goodman A.A.</name></creator><date role="Updated">2011-05-30T07:36:32Z</date><date role="Created">2011-05-16T14:49:40Z</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>interstellar-medium</subject><subject>molecular-clouds</subject><subject>young-stellar-objects</subject><description>We present the chemistry, temperature, and dynamical state of a sample of 193 dense cores or core candidates in the Perseus Molecular cloud and compare the properties of cores associated with young stars and clusters with those which are not. The combination of our NH3 and CCS observations with previous millimeter, submillimeter, and Spitzer data available for this cloud enables us both to determine core properties precisely and to accurately classify cores as starless or protostellar.</description><source format="bibcode">2009ApJ...696..298F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/696/298</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/175/509">J/ApJS/175/509 : Ammonia spectral atlas in Perseus (Rosolowsky+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/684/1240">J/ApJ/684/1240 : Prestellar cores in Perseus, Serpens and Ophiuchus (Enoch+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/468/1009">J/A+A/468/1009 : Star formation in Perseus. 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