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<ri:Resource created="2024-04-17T08:52:22Z" status="active" updated="2025-08-21T20:01:04Z" 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>Ammonia observations of Planck cold cores</title><shortName>J/A+A/684/A144</shortName><identifier>ivo://CDS.VizieR/J/A+A/684/A144</identifier><altIdentifier>doi:10.26093/cds/vizier.36840144</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Berdikhan D.</name></creator><creator><name>Esimbek J.</name></creator><creator><name>Henkel C.</name></creator><creator><name>Zhou J.</name></creator><creator><name>Tang X.</name></creator><creator><name>Liu T.</name></creator><creator><name>Wu G.</name></creator><creator><name>Li D.,He Y.</name></creator><creator><name>Komesh T.</name></creator><creator><name>Tursun K.</name></creator><creator><name>Zhou D.</name></creator><creator><name>Imanaly E.</name></creator><creator><name>Jandaolet Q.</name></creator><date role="Updated">2025-08-21T20:01:04Z</date><date role="Created">2024-04-17T08:52:22Z</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>radial-velocity</subject><subject>radio-astronomy</subject><subject>surveys</subject><description>Single-pointing observations of NH_3_(1,1) and (2,2) were conducted toward 672 Planck Early Cold Cores (ECCs) using the Nanshan 26-m radio telescope. Out of these sources, a detection rate of 37 (249 cores) was achieved, with a NH_3_(1,1) hyperfine structure detected in 187 cores and NH_3_(2,2) emission lines detected in 76 of them. The detection rate of NH_3_ is positively correlated with the continuum emission fluxes at a frequency of 857GHz. Among the observed 672 cores, ~22 have associated stellar and infrared objects within the beam size (~2 arcmin). This suggests that most of the cores in our sample may be starless. The kinetic temperatures of the cores range from 8.9 to 20.7K, with an average of 12.3K, indicating a coupling between gas and dust temperatures. The ammonia column densities range from 3.6*10^14^ to 6.07*10^15^cm^-2^, with a median value of 2.04*10^15cm^-2^. The fractional abundances of ammonia range from 0.3 to 9.7*10^-7^, with an average of 2.7*10^-7^, which is one order of magnitude larger than that of massive star-forming (MSF) regions and infrared dark clouds (IRDCs). The correlation between thermal and nonthermal velocity dispersion of the NH_3_(1,1) inversion transition indicates the dominance of supersonic nonthermal motions in the dense gas traced by NH3, and the relationship between these two parameters in Planck cold cores is weaker, with lower values observed for both parameters relative to other samples under our examination. The cumulative distribution shapes of line widths in the Planck cold cores closely resemble those of the dense cores found in regions of Cepheus, in addition to Orion L1630 and L1641, with higher values compared to Ophiuchus.</description><source format="bibcode">2024A&amp;A...684A.144B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/684/A144</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></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/684/A144</accessURL><mirrorURL title="VizieR at IUCAA: 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LSR velocity of the NH_3_(2,2) inversion transition (23.722GHz)</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_v(22)</name><description>? rms uncertainty on v(2,2)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dv(22)</name><description>? NH_3_(2,2) linewidth</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_dv(22)</name><description>? rms uncertainty on dv(2,2)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>TMB(22)</name><description>? 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LSR velocity of the C^18^O(1-0) line</description><unit>km/s</unit><ucd>spect.dopplerVeloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_vC18O</name><description>? rms uncertainty on v13CO</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dvC18O</name><description>? C^18^O linewidth</description><unit>km/s</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_dvC18O</name><description>? rms uncertainty on dvC18O</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>TMBC18O</name><description>? Main beam brightness temperature of the C^18^O(1-0) transition</description><unit>K</unit><ucd>phys.temperature;meta.main</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_TMBC18O</name><description>? rms uncertainty on TMBC18O</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/A+A/684/A144/tablec2</name><description>Derived parameters of CO line</description><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>Galactic name (GLLL.ll+BB.bb)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>Tex(CO)</name><description>Excitation temperature derived from CO lines</description><unit>K</unit><ucd>phys.atmol.excitation</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Tex(CO)</name><description>rms uncertainty on Tex(CO)</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>tau(13CO)</name><description>? Optical depth of ^13^CO</description><ucd>phys.absorption.opticalDepth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_tau(13CO)</name><description>? rms uncertainty on tau(13CO)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>tau(C18O)</name><description>? Optical depth of C^18^O</description><ucd>phys.absorption.opticalDepth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_tau(C18O)</name><description>? rms uncertainty on tau(C18O)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>N(13CO)</name><description>? ^13^CO column density N(13CO)</description><unit>log(cm**-2)</unit><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_N(13CO)</name><description>? rms uncertainty on N(13CO)</description><unit>log(cm**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>N(C18O)</name><description>? ^13^CO column density N(C18O)</description><unit>log(cm**-2)</unit><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_N(C18O)</name><description>? rms uncertainty on N(C18O)</description><unit>log(cm**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NH2(13CO)</name><description>? Hydrogen column density derived from ^13C^O column density</description><unit>log(cm**-2)</unit><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_NH2(13CO)</name><description>? rms uncertainty on NH2(13CO)</description><unit>log(cm**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>NH2(C18O)</name><description>? Hydrogen column density derived from C^18^O column density</description><unit>log(cm**-2)</unit><ucd>phys.columnDensity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_NH2(C18O)</name><description>? rms uncertainty on NH2(C18O)</description><unit>log(cm**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>