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<ri:Resource created="2017-01-16T12:58:09Z" 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>Molecular clouds in the Milky Way with CO obs.</title><shortName>J/ApJ/828/59</shortName><identifier>ivo://CDS.VizieR/J/ApJ/828/59</identifier><altIdentifier>doi:10.26093/cds/vizier.18280059</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Su Y.</name></creator><creator><name>Sun Y.</name></creator><creator><name>Li C.</name></creator><creator><name>Zhang S.</name></creator><creator><name>Zhou X.</name></creator><creator><name>Fang M.</name></creator><creator><name>Yang J.</name></creator><creator><name>Chen X.</name></creator><date role="Updated">2017-03-01T13:09:14Z</date><date role="Created">2017-01-16T12:58:09Z</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>milky-way-galaxy</subject><subject>radio-astronomy</subject><subject>surveys</subject><description>The Galactic plane has been mapped from l=34.75{deg} to 45.25{deg} and b=-5.25{deg} to 5.25{deg} in the CO (J=1-0) emission with the 13.7m telescope of the Purple Mountain Observatory. The unbiased survey covers a large area of 110 square degrees sampled every 30" with a velocity resolution of ~0.2km/s. In this paper, we present the result of an unbiased CO survey of this longitude and latitude range in the velocity range from -60 to -10km/s. Over 500 molecular clouds (MCs) are picked out from the ^12^CO (J=1-0) emission, and 131 of these MCs are associated with ^13^CO emission. The distant MCs, which lie beyond the solar circle and are mostly concentrated in the Galactic plane, trace the large-scale molecular gas structure over 10 degrees of Galactic azimuth. We find that the distribution of the distant MCs can be well fitted by a Gaussian function with a full width at half maximum (FWHM) of 0.7{deg} with the Galactic latitude. We suggest that the CO emission of the segment is from the Outer Arm. The physical mid-plane traced by the Outer Arm seems to be slightly displaced from the IAU-defined plane on a large scale, which could be explained by the warped plane at large Galactocentric distances of &gt;~10kpc and the apparent tilted mid-plane to the projected IAU-defined plane caused by the Sun's z-height above the disk for distances near and within the Solar circle. After removing the effect of the warp and tilted structure, the scale height of the MCs in the Outer Arm is about 0.6{deg} or 160pc at a heliocentric distance of 15kpc. If the inner plane of our Galaxy is flat, we can derive an upper limit of the Sun's offset of ~17.1pc above the physical mid-plane of the Milky Way. We also discuss the correlations between the physical parameters of the distant MCs, which is quite consistent with the result of other studies of this parameter.</description><source format="bibcode">2016ApJ...828...59S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/828/59</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/40">VIII/40 : GB6 catalog of radio sources (Gregory+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/58">VIII/58 : A Survey of Radio H II Regions in the Northern Sky (Lockman+ 1989)</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/ApJS/224/7">J/ApJS/224/7 : CO obs. of the outer arm in the 2nd quadrant (Du+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/221/26">J/ApJS/221/26 : Radio obs. of Galactic WISE HII regions (Anderson+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/798/L27">J/ApJ/798/L27 : CO obs. of molecular clouds in the 2nd quadrant (Sun+, 2015)</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/AJ/147/46">J/AJ/147/46 : Properties of clumps in the NAN complex (Zhang+, 2014)</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/ApJS/194/32">J/ApJS/194/32 : The HII Region Discovery Survey (HRDS). 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