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<ri:Resource created="2014-05-07T07:26:39Z" 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>A 3mm line survey in 37 IR dark clouds</title><shortName>J/ApJ/756/60</shortName><identifier>ivo://CDS.VizieR/J/ApJ/756/60</identifier><altIdentifier>doi:10.26093/cds/vizier.17560060</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sanhueza P.</name></creator><creator><name>Jackson J.M.</name></creator><creator><name>Foster J.B.</name></creator><creator><name>Garay G.</name></creator><creator><name>Silva A.</name></creator><creator><name>Finn S.C.</name></creator><date role="Updated">2017-06-01T08:52:28Z</date><date role="Created">2014-05-07T07:26:39Z</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>chemical-abundances</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><subject>molecular-clouds</subject><subject>interstellar-medium</subject><description>We have observed 37 Infrared Dark Clouds (IRDCs), containing a total of 159 clumps, in high-density molecular tracers at 3mm using the 22m ATNF Mopra Telescope located in Australia. After determining kinematic distances, we eliminated clumps that are not located in IRDCs and clumps with a separation between them of less than one Mopra beam. Our final sample consists of 92 IRDC clumps. The most commonly detected molecular lines are (detection rates higher than 8%) N_2_H^+^, HNC, HN^13^C, HCO^+^, H^13^CO^+^, HCN, C_2_H, HC_3_N, HNCO, and SiO. We investigate the behavior of the different molecular tracers and look for chemical variations as a function of an evolutionary sequence based on Spitzer IRAC and MIPS emission. Optical depth calculations show that in IRDC clumps the N_2_H^+^ line is optically thin, the C_2_ H line is moderately optically thick, and HNC and HCO^+^ are optically thick.</description><source format="bibcode">2012ApJ...756...60S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/756/60</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/J/A+A/530/A118">J/A+A/530/A118 : G29.96-0.02 and G35.20-1.74 1mm and 3mm maps (Pillai+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/527/A88">J/A+A/527/A88 : Chemistry in infrared dark clouds (Vasyunina+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/197/25">J/ApJS/197/25 : MALT90 pilot survey (Foster+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/715/310">J/ApJ/715/310 : Early stages of star formation in IRDCs (Rathborne+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/710/150">J/ApJ/710/150 : Molecular lines in EGOs (Chen+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/515/A42">J/A+A/515/A42 : Catalog of high extinction clouds (Rygl+, 2010)</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/MNRAS/399/1506">J/MNRAS/399/1506 : IRDC cores in SCUBA Legacy Catalogue (Parsons+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/2391">J/AJ/136/2391 : GLIMPSE Extended Green Objects catalog (Cyganowski+, 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/PAZh/33/143">J/PAZh/33/143 : Laboratory studies of HNCO (Lapinov+, 2007)</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/651/L125">J/ApJ/651/L125 : Water masers associated with IR dark cloud cores (Wang+, 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/A+A/432/369">J/A+A/432/369 : Leiden Atomic and Molecular Database (LAMDA) 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