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<ri:Resource created="2012-11-13T13:26:42Z" 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>Planck cold dust clumps CO survey</title><shortName>J/ApJ/756/76</shortName><identifier>ivo://CDS.VizieR/J/ApJ/756/76</identifier><altIdentifier>doi:10.26093/cds/vizier.17560076</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Wu Y.</name></creator><creator><name>Liu T.</name></creator><creator><name>Meng F.</name></creator><creator><name>Li D.</name></creator><creator><name>Qin S.-L.</name></creator><creator><name>Ju B.-G.</name></creator><date role="Updated">2017-07-10T06:21:50Z</date><date role="Created">2012-11-13T13:26:42Z</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>interstellar-medium</subject><subject>radio-astronomy</subject><subject>molecular-clouds</subject><description>A survey toward 674 Planck cold clumps of the Early Cold Core Catalogue (ECC) in the J=1-0 transitions of ^12^CO, ^13^CO, and C^18^O has been carried out using the Purple Mountain Observatory 13.7m telescope. Six hundred seventy-three clumps were detected with ^12^CO and ^13^CO emission, and 68% of the sample has C^18^O emission. Additional velocity components were also identified. A close consistency of the three line peak velocities was revealed for the first time. Kinematic distances are given for all the velocity components, and half of the clumps are located within 0.5 and 1.5kpc. Excitation temperatures range from 4 to 27K, slightly larger than those of T_d_. Line width analysis shows that the majority of ECC clumps are low-mass clumps. Ten clumps were mapped. Twelve velocity components and 22 cores were obtained. Their morphologies include extended diffuse, dense, isolated, cometary, and filament, of which the last is the majority. Twenty cores are starless, and only seven cores seem to be in a gravitationally bound state. Planck cold clumps are the most quiescent among the samples of weak red IRAS, infrared dark clouds, UC HII candidates, extended green objects, and methanol maser sources, suggesting that Planck cold clumps have expanded the horizon of cold astronomy.</description><source format="bibcode">2012ApJ...756...76W</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/756/76</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/VIII/88">VIII/88 : Planck Early Release Compact Source Catalogue (Planck, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/244">VII/244 : Atlas and Catalog of Dark Clouds (Dobashi+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/39">VIII/39 : Composite CO Survey of the Milky Way (Dame+ 1987)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/20">VII/20 : Catalogue of HII Regions (Sharpless 1959)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/202/4">J/ApJS/202/4 : Planck cold clumps survey in the Orion complex (Liu+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/710/150">J/ApJ/710/150 : Molecular lines in EGOs (Chen+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/686/384">J/ApJ/686/384 : ^12^CO, ^13^CO, C^18^O survey of IRDCs (Du+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/391/869">J/MNRAS/391/869 : A mapping survey of massive CO cores (Guan+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/641/389">J/ApJ/641/389 : Millimetric observations of IRDC cores (Rathborne+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/653/1325">J/ApJ/653/1325 : Galactic distribution of infrared dark clouds (Simon+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/152/81">J/ApJS/152/81 : CO survey toward starless cores (Park+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/566/945">J/ApJ/566/945 : Massive star forming regions at 1.2mm (Beuther+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/380/665">J/A+A/380/665 : Massive dense cores with ^13^CO J=1-0 lines (Wu+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/308/573">J/A+A/308/573 : Ammonia on YSOs IRAS sources (Molinari+ 1996)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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Antenna temperature for ^12^CO</description><unit>K</unit><ucd>phot.antennaTemp;em.line.CO;spect.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Source name (GLLL.ll+BB.bb)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>V12</name><description>? Local Standard of Rest velocity for ^12^CO</description><unit>km/s</unit><ucd>spect.dopplerVeloc;em.line.CO</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_V12</name><description>? 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