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<ri:Resource created="2017-06-12T09:39:22Z" status="active" updated="2025-08-29T20:10:29Z" 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>Milky Way molecular clouds from ^12^CO</title><shortName>J/ApJ/834/57</shortName><identifier>ivo://CDS.VizieR/J/ApJ/834/57</identifier><altIdentifier>doi:10.26093/cds/vizier.18340057</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Miville-Deschenes M.-A.</name></creator><creator><name>Murray N.</name></creator><creator><name>Lee E.J.</name></creator><date role="Updated">2025-08-29T20:10:29Z</date><date role="Created">2017-06-12T09:39:22Z</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>molecular-clouds</subject><subject>co-line-emission</subject><subject>galaxy-planes</subject><subject>milky-way-galaxy</subject><subject>interstellar-medium</subject><description>This study presents a catalog of 8107 molecular clouds that covers the entire Galactic plane and includes 98% of the ^12^CO emission observed within b+/-5^{deg}^. The catalog was produced using a hierarchical cluster identification method applied to the result of a Gaussian decomposition of the Dame+ (2001ApJ...547..792D) data. The total H_2_ mass in the catalog is 1.2x10^9^M_{sun}_, in agreement with previous estimates. We find that 30% of the sight lines intersect only a single cloud, with another 25% intersecting only two clouds. The most probable cloud size is R~30pc. We find that M{propto}R^2.2+/-0.2^, with no correlation between the cloud surface density, {Sigma}, and R. In contrast with the general idea, we find a rather large range of values of {Sigma}, from 2 to 300M_{sun}_/pc^2^, and a systematic decrease with increasing Galactic radius, R_gal_. The cloud velocity dispersion and the normalization {sigma}_0_={sigma}_v_/R^1/2^ both decrease systematically with R_gal_. When studied over the whole Galactic disk, there is a large dispersion in the line width-size relation and a significantly better correlation between {sigma}_v_ and {Sigma}R. The normalization of this correlation is constant to better than a factor of two for R_gal_&lt;20kpc. This relation is used to disentangle the ambiguity between near and far kinematic distances. We report a strong variation of the turbulent energy injection rate. In the outer Galaxy it may be maintained by accretion through the disk and/or onto the clouds, but neither source can drive the 100 times higher cloud-averaged injection rate in the inner Galaxy.</description><source format="bibcode">2017ApJ...834...57M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/834/57</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/39">VIII/39 : Composite CO Survey of the Milky Way (Dame+ 1987)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/833/229">J/ApJ/833/229 : Star forming cloud-GMC complexes (Lee+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/590/A131">J/A+A/590/A131 : Giant molecular filaments in the MW (Abreu-Vicente+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/738/27">J/ApJ/738/27 : Galactic HII regions RRL and continuum data (Balser+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/734/65">J/ApJ/734/65 : CI radial velocities with HST/STIS (Jenkins+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/723/492">J/ApJ/723/492 : Properties of GRS molecular clouds (Roman-Duval+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/184/1">J/ApJS/184/1 : Molecular clouds in the LMC by NANTEN. II. (Kawamura+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/699/1153">J/ApJ/699/1153 : Kinematic dist. to GRS molecular clouds (Roman-Duval+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/699/1092">J/ApJ/699/1092 : Giant molecular clouds (SRBY) (Heyer+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/182/131">J/ApJS/182/131 : Molecular clouds and clumps in the GRS (Rathborne+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/686/948">J/ApJ/686/948 : CO in extragalactic giant molecular clouds (Bolatto+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/144/47">J/ApJS/144/47 : Outer galaxy molecular cloud catalog (Brunt+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/582/756">J/ApJ/582/756 : Velocities of HII regions (Kolpak+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/551/852">J/ApJ/551/852 : FCRAO CO survey of the outer 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