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<ri:Resource created="2015-04-30T14:15:48Z" 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>Orion A dense cores based on 1.1mm and C^18^O</title><shortName>J/ApJS/217/7</shortName><identifier>ivo://CDS.VizieR/J/ApJS/217/7</identifier><altIdentifier>doi:10.26093/cds/vizier.22170007</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Shimajiri Y.</name></creator><creator><name>Kitamura Y.</name></creator><creator><name>Nakamura F.</name></creator><creator><name>Momose M.</name></creator><creator><name>Saito M.</name></creator><creator><name>Tsukagoshi T.,Hiramatsu M.</name></creator><creator><name>Shimoikura T.</name></creator><creator><name>Dobashi K.</name></creator><creator><name>Hara C.</name></creator><creator><name>Kawabe R.</name></creator><date role="Updated">2017-12-04T08:52:20Z</date><date role="Created">2015-04-30T14:15:48Z</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>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><subject>interstellar-medium</subject><description>We present Orion A giant molecular cloud core catalogs, which are based on a 1.1mm map with an angular resolution of 36" (~0.07pc) and C^18^O (J=1-0) data with an angular resolution of 26.4" (~0.05pc). We have cataloged 619 dust cores in the 1.1mm map using the Clumpfind method. The ranges of the radius, mass, and density of these cores are estimated to be 0.01-0.20pc, 0.6-1.2x10^2^M_{sun}_ , and 0.3x10^4^-9.2x10^6^cm^-3^, respectively. We have identified 235 cores from the C^18^O data. The ranges of the radius, velocity width, LTE mass, and density are 0.13-0.34pc, 0.31-1.31km/s, 1.0-61.8M_{sun}_ , and (0.8-17.5)x10^3^cm^-3^, respectively. From the comparison of the spatial distributions between the dust and C^18^O cores, four types of spatial relations were revealed: (1) the peak positions of the dust and C^18^O cores agree with each other (32.4% of the C^18^O cores), (2) two or more C^18^O cores are distributed around the peak position of one dust core (10.8% of the C^18^O cores), (3) 56.8% of the C^18^O cores are not associated with any dust cores, and (4) 69.3% of the dust cores are not associated with any C^18^O cores.</description><source format="bibcode">2015ApJS..217....7S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/217/7</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/244">VII/244 : Atlas and Catalog of Dark Clouds (Dobashi+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/564/A68">J/A+A/564/A68 : Orion A GMC 13CO and C18O maps (Shimajiri+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/192">J/AJ/144/192 : Spitzer survey of Orion A and B. I. YSOs (Megeath+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/202/4">J/ApJS/202/4 : Planck cold clumps survey in the Orion complex (Liu+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/732/101">J/ApJ/732/101 : C^18^O cores in the S140 cloud (Ikeda+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/496/153">J/A+A/496/153 : Molecular hydrogen flows along Ori A cloud (Davis+, 2009)</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/MNRAS/374/1413">J/MNRAS/374/1413 : SCUBA survey of Orion (Nutter+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/665/1194">J/ApJ/665/1194 : Dense cores in the Orion A cloud survey (Ikeda+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/655/351">J/ApJ/655/351 : Massive quiescent cores in Orion. II. 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