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<ri:Resource created="2014-11-19T14:21:31Z" 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>First quadrant IRDCs in CS(2-1) with Mopra</title><shortName>J/ApJ/764/102</shortName><identifier>ivo://CDS.VizieR/J/ApJ/764/102</identifier><altIdentifier>doi:10.26093/cds/vizier.17640102</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Finn S.C.</name></creator><creator><name>Jackson J.M.</name></creator><creator><name>Rathborne J.M.</name></creator><creator><name>Chambers E.T.</name></creator><creator><name>Simon R.</name></creator><date role="Updated">2014-12-06T08:51:02Z</date><date role="Created">2014-11-19T14:21:31Z</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>radio-astronomy</subject><subject>infrared-sources</subject><subject>milky-way-galaxy</subject><description>Infrared dark clouds (IRDCs) are believed to host the earliest stages of high-mass star and cluster formation. Because O stars typically travel short distances over their lifetimes, if IRDCs host the earliest stages of high-mass star formation then these cold, dense molecular clouds should be located in or near the spiral arms in the Galaxy. The Galactic distribution of a large sample of IRDCs should therefore provide information on Galactic structure. Moreover, determination of distances enables mass and luminosity calculations. We have observed a large sample of IRDC candidates in the first Galactic quadrant in the dense gas tracer CS(2-1) using the Mopra telescope in order to determine kinematic distances from the molecular line velocities. We find that the IRDCs are concentrated around a Galactocentric distance of ~4.5kpc, agreeing with the results of Simon et al. (2006, J/ApJ/653/1325). This distribution is consistent with the location of the Scutum-Centaurus spiral arm. The group of IRDCs near the Sun in the first quadrant detected in ^13^CO(1-0) in Simon et al. is not detected in the CS data. This discrepancy arises from the differences in the critical densities between the ^13^CO(1-0) and CS(2-1) lines. We determine that the Midcourse Space Experiment selected IRDCs are not a homogeneous population, and ^13^CO(1-0) traces a population of IRDCs with lower column densities and lower 1.1 mm flux densities in addition to more dense IRDCs detected in CS. Masses of the first quadrant IRDCs are calculated from ^13^CO(1-0) maps. We find a strong peak in the Galactocentric IRDC mass surface density distribution at R_Gal_~4.5kpc.</description><source format="bibcode">2013ApJ...764..102F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/764/102</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/293">II/293 : GLIMPSE Source Catalog (I + II + 3D) (IPAC 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/559/A79">J/A+A/559/A79 : IRDC APEX/SABOCA observations (Ragan+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/754/62">J/ApJ/754/62 : HRDS III. HII region kinematic distances (Anderson+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/721/137">J/ApJ/721/137 : The Bolocam Galactic Plane Survey (BGPS) (Bally+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/399/1506">J/MNRAS/399/1506 : IRDC cores in SCUBA Legacy Catalogue (Parsons+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/505/405">J/A+A/505/405 : A catalogue of Spitzer dark clouds (Peretto+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/499/149">J/A+A/499/149 : 1.2mm maps of southern Infrared Dark Clouds (Vasyunina+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/686/384">J/ApJ/686/384 : ^12^CO, ^13^CO, C^18^O survey of IRDCs (Du+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/680/349">J/ApJ/680/349 : Galactic distribution of IRDCs (Jackson+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/653/1325">J/ApJ/653/1325 : Galactic distribution of infrared dark clouds (Simon+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/641/389">J/ApJ/641/389 : Millimetric observations of IRDC cores (Rathborne+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/639/227">J/ApJ/639/227 : MSX IRDC candidate catalog (Simon+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/566/945">J/ApJ/566/945 : Massive star forming regions at 1.2mm (Beuther+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/358/257">J/A+A/358/257 : Molecular clouds SO and CS obs. 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