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<ri:Resource created="2009-11-05T21:27:48Z" 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>Starless cores in HCN(J=1-0)</title><shortName>J/ApJ/664/928</shortName><identifier>ivo://CDS.VizieR/J/ApJ/664/928</identifier><altIdentifier>doi:10.26093/cds/vizier.16640928</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sohn J.</name></creator><creator><name>Lee C.W.</name></creator><creator><name>Park Y.-S.</name></creator><creator><name>Lee H.M.</name></creator><creator><name>Myers P.C.</name></creator><creator><name>Lee Y.</name></creator><date role="Updated">2017-10-16T14:57:40Z</date><date role="Created">2009-11-05T21:27:48Z</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-clouds</subject><subject>interstellar-medium</subject><subject>radio-astronomy</subject><description>We have carried out a survey toward the central regions of 85 starless cores in HCN(J=1-0) to study inward motions in the cores. Sixty-four cores were detected with HCN lines. The infall asymmetry in the HCN spectra is found to be more prevalent, and more prominent than in any other previously used infall tracers such as CS(J=2-1), DCO^+^(J=2-1), and N2H^+^(J=1-0). 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>n_Name</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Name</name><description>Source name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType><flag>primary</flag></column><column><name>f_Name</name><description>[a] double peaked sources (1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>T.HCN</name><description>Antenna temperature of HCN J=1-0 (F=2-1)</description><unit>K</unit><ucd>phot.antennaTemp</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_T.H13CN</name><description>The 3{sigma} limit flag on T.H13CN</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>T.H13CN</name><description>? 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Error in V(F=1-1)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>V(F=2-1)</name><description>? Peak HCN J=1-0(F=2-1) intensity velocity</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_V(F=2-1)</name><description>? Error in V(F=2-1)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>VN2H</name><description>? The N_2_H+ velocity (3)</description><unit>km/s</unit><ucd>spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_VN2H</name><description>? 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