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<ri:Resource created="2006-10-01T11:58:51Z" 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>Observations at 850um in Perseus clusters</title><shortName>J/A+A/440/151</shortName><identifier>ivo://CDS.VizieR/J/A+A/440/151</identifier><altIdentifier>doi:10.26093/cds/vizier.34400151</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hatchell J.</name></creator><creator><name>Richer J.S.</name></creator><creator><name>Fuller G.A.</name></creator><creator><name>Qualtrough C.J.</name></creator><creator><name>Ladd E.F.,Chandler C.J.</name></creator><date role="Updated">2006-10-01T12:02:54Z</date><date role="Created">2006-10-01T11:58:51Z</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>molecular-clouds</subject><subject>radio-spectroscopy</subject><description>We present a complete survey of current star formation in the Perseus molecular cloud, made at 850 and 450{mu} with SCUBA at the JCMT. Covering 3deg^2^, this submillimetre continuum survey for protostellar activity is second in size only to that of rho Ophiuchus (Johnstone et al., 2004ApJ...611L..45J). Complete above 0.4M_{sun}_ (5{sigma} detection in a 14" beam), we detect a total of 91 protostars and pre-stellar cores. Of these, 80% lie in clusters, representative of star formation across the Galaxy. Two of the groups of cores are associated with the young stellar clusters IC 348 and NGC 1333, and are consistent with a steady or reduced star formation rate in the last 0.5Myr, but not an increasing one. In Perseus, 40-60% of cores are in small clusters (&lt;50M_{sun}_) and isolated objects, much more than the 10% suggested from infrared studies. Complementing the dust continuum, we present a C^18^O map of the whole cloud at 1' resolution.</description><source format="bibcode">2005A&amp;A...440..151H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/440/151</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/A+A/359/113">J/A+A/359/113 : X-ray and IR study of Rho Oph dark cloud (Grosso+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/55/653">J/PASJ/55/653 : Chandra X-ray flares in rho Ophiuchi (Imanishi+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/429/963">J/A+A/429/963 : XMM-Newton observation of the rho Oph cloud (Ozawa+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/430/549">J/A+A/430/549 : C^18^O/C^17^O near rho Oph (Wouterloot+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/630/381">J/ApJ/630/381 : Mid-IR imaging in {rho} Oph (Barsony+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/447/609">J/A+A/447/609 : mm continuum obs. in rho Oph cloud (Stanke+, 2006)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/440/151</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/440/151</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/440/151</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/440/151</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/440/151</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/440/151</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/A+A/440/151/tablea1 (SCUBA 850{mu}m core positions, names and references, peak 850{mu}m fluxes and C^18^O integrated intensity at the submm peak position)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/440/151/tablea1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/440/151/tablea1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/440/151/tablea1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>53.324583</ra><dec>31.159167</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/857-860 862 881 1539 1542</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/440/151?format=ascii</footprint><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/440/151/tablea1</name><description>SCUBA 850{mu}m core positions, names and references, peak 850{mu}m fluxes and C^18^O integrated intensity at the submm peak position</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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