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<ri:Resource created="2022-12-06T09:33:00Z" status="active" updated="2025-06-13T15:25:00Z" 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>Column density maps for MWISP ^13^CO mol. clouds</title><shortName>J/ApJS/262/16</shortName><identifier>ivo://CDS.VizieR/J/ApJS/262/16</identifier><altIdentifier>doi:10.26093/cds/vizier.22620016</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ma Y.</name></creator><creator><name>Wang H.</name></creator><creator><name>Zhang M.</name></creator><creator><name>Wang C.</name></creator><creator><name>Zhang S.</name></creator><creator><name>Liu Y.</name></creator><creator><name>Li C.</name></creator><creator><name>Zheng Y.,Yuan L.</name></creator><creator><name>Yang Ji</name></creator><date role="Updated">2022-12-12T13:28:47Z</date><date role="Created">2022-12-06T09:33:00Z</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>interstellar-medium</subject><subject>surveys</subject><subject>co-line-emission</subject><subject>molecular-physics</subject><subject>milky-way-galaxy</subject><description>We have obtained column density maps for an unbiased sample of 120 molecular clouds in the third quadrant of the Milky Way midplane (b&lt;=|5|{deg}) within the Galactic longitude range from 195{deg} to 225{deg}, using the high-sensitivity ^12^CO and ^13^CO (J=1-0) data from the Milky Way Imaging Scroll Painting (MWISP) project. The probability density functions of the molecular hydrogen column density of the clouds, N-pdfs, are fitted with both a lognormal (LN) function and a lognormal plus power-law (LN+PL) function. The molecular clouds are classified into three categories according to their shapes of N-pdfs, i.e., LN, LN+PL, and UN (unclear). About 72% of the molecular clouds fall into the LN category, while 18% and 10% fall into the LN+PL and UN categories, respectively. A PL scaling relation, {sigma}_s_{propto}N_H2_^0.44^, exists between the width of the N-pdf, {sigma}_s_, and the average column density, N_H2_, of the molecular clouds. However, {sigma}_s_ shows no correlation with the mass of the clouds. A correlation is found between the dispersion of normalized column density, {sigma}_N/&lt;N&gt;_, and the sonic Mach number, M, of molecular clouds. Overall, as predicted by numerical simulations, the N-pdfs of the molecular clouds with active star formation activity tend to have N-pdfs with PL high-density tails.</description><source format="bibcode">2022ApJS..262...16M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/262/16</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/II/360">II/360 : Gaia DR2 x AllWISE catalogue (Marton+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/20">VII/20 : Catalogue of HII Regions (Sharpless 1959)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/284">VII/284 : A Catalogue of Galactic Supernova Remnants (Green, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/551/852">J/ApJ/551/852 : FCRAO CO survey of the outer Galaxy (Heyer+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/487/993">J/A+A/487/993 : MAMBO Mapping of c2d Clouds and Cores (Kauffmann+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/560/A24">J/A+A/560/A24 : IRAM 30m CO-observations in W43 (Carlhoff+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/212/1">J/ApJS/212/1 : The WISE catalog of Galactic HII regions (Anderson+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/783/130">J/ApJ/783/130 : Parallaxes of high mass star forming regions (Reid+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/578/A29">J/A+A/578/A29 : Column density maps in 4 IRDCs (Schneider+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/458/3479">J/MNRAS/458/3479 : SVM selection of WISE YSO Candidates (Marton+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/834/57">J/ApJ/834/57 : MW molecular clouds from ^12^CO (Miville-Deschenes+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/878/44">J/ApJ/878/44 : ^13^CO clumps toward the Cas A supernova remnant (Ma+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/633/A147">J/A+A/633/A147 : FQS. Galactic Plane CO survey (Benedettini+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/254/3">J/ApJS/254/3 : CO obs. of molecular clouds in the MW midplane (Ma+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/257/51">J/ApJS/257/51 : Morphologies of MWISP ^12^CO mol. 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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>MWISP</name><description>MWISP designation (GLLL.lll+BB.bbb+vvv.vv) (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="22*">char</dataType></column><column><name>Fig</name><description>Figure number; column added by CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>_Glon</name><description>Positions from MWISP names (longitude part)</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>_Glat</name><description>Positions from MWISP names (latitude part)</description><unit>deg</unit><ucd>pos.galactic.lat</ucd></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>Dist</name><description>Distance of the cloud</description><unit>kpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>mu</name><description>[-1.74/0.65]? Fit parameter, {mu}, of the N-pdfs in Equations 5-6 (Section 3.2.1)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>sigS</name><description>[0.58/2.63]? Fit parameter, {sigma}_S_, of the N-pdfs in Equations 5-6 (Section 3.2.1)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>br</name><description>[0.26/1.9]? 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Radius</description><unit>pc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Mass</name><description>[0/50552]? 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