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<ri:Resource created="2023-12-22T15:08:03Z" 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>CO obs. of molecular clouds in the 3rd Gal. quadrant</title><shortName>J/ApJS/268/1</shortName><identifier>ivo://CDS.VizieR/J/ApJS/268/1</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dong Y.</name></creator><creator><name>Sun Y.</name></creator><creator><name>Xu Ye</name></creator><creator><name>Lin Z.</name></creator><creator><name>Bian S.</name></creator><creator><name>Hao C.</name></creator><creator><name>Liu D.</name></creator><creator><name>Li Y.</name></creator><creator><name>Yang Ji,Su Y.</name></creator><creator><name>Zhou X.</name></creator><creator><name>Zhang S.</name></creator><creator><name>Yan Q.-Z.</name></creator><creator><name>Chen Z.</name></creator><date role="Updated">2024-11-12T11:24:54Z</date><date role="Created">2023-12-22T15:08:03Z</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>milky-way-galaxy</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><description>We present the results of an unbiased 12CO/13CO/C18O (J=1-0) survey in a portion of the third Galactic quadrant (TGQ): 219.75{deg}&lt;=l&lt;=229.75{deg} and -5.25{deg}&lt;=b&lt;=5.25{deg}. The high-resolution and high-sensitivity data sets help to unravel the distributions and physical properties of the molecular clouds (MCs) in the mapped area. In the LSR velocity range from ~-1 to ~85km/s, the molecular material successfully traces the Local, Perseus, and Outer arms. In the TGQ, the Outer arm appears to be more prominent than that in the second Galactic quadrant (SGQ), but the Perseus arm is not as conspicuous as that in the SGQ. A total of 1502 ^12^CO, 570 ^13^CO, and 53 C^18^O molecular structures are identified, spanning over ~2 and ~6 orders of magnitude in size and mass, respectively. Tight mass-radius correlations and virial parameter-mass anticorrelations are observable. Yet, it seems that no clear correlations between velocity dispersion and effective radius can be found over the full dynamic range. The vertical distribution of the MCs renders evident pictures of the Galactic warp and flare.</description><source format="bibcode">2023ApJS..268....1D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/268/1</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/VII/50">VII/50 : CO Radial Velocities Toward Galactic H II Regions (Blitz+ 1982)</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/J/A+A/327/325">J/A+A/327/325 : Distances of molecular cloud (May+, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/127/181">J/A+AS/127/181 : H2O maser sources new detections (Han+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/368/845">J/A+A/368/845 : Arcetri Cat. of H2O maser sources (Valdettaro+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/397/133">J/A+A/397/133 : Star-forming complexes in the Galaxy (Russeil+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/56/313">J/PASJ/56/313 : 13CO survey of Mon &amp; CMa molecular clouds (Kim+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/59/1185">J/PASJ/59/1185 : Water maser in galactic IRAS sources (Sunada+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/672/930">J/ApJ/672/930 : Distant CO clouds in 3rd Galactic quadrant (Vazquez+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/723/492">J/ApJ/723/492 : GRS molecular clouds (Roman-Duval+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/418/1689">J/MNRAS/418/1689 : Red MSX water maser and ammonia emissions (Urquhart+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/772/45">J/ApJ/772/45 : Hi-GAL obs.: star formation in 3rd quadrant (Elia+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/431/1752">J/MNRAS/431/1752 : ATLASGAL 6.7GHz methanol masers (Urquhart+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/435/400">J/MNRAS/435/400 : ATLASGAL. 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