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<ri:Resource created="2020-02-06T15:37:20Z" 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>Massive star-forming clump from MALT90</title><shortName>J/ApJS/243/13</shortName><identifier>ivo://CDS.VizieR/J/ApJS/243/13</identifier><altIdentifier>doi:10.26093/cds/vizier.22430013</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Li M.</name></creator><creator><name>Zhou J.</name></creator><creator><name>Esimbek J.</name></creator><creator><name>Quan D.</name></creator><creator><name>He Y.</name></creator><creator><name>Li Q.</name></creator><creator><name>Zhu C.</name></creator><date role="Updated">2021-02-23T10:45:30Z</date><date role="Created">2020-02-06T15:37:20Z</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>star-forming-regions</subject><subject>interstellar-medium</subject><subject>radio-astronomy</subject><description>We selected 90 massive star-forming clumps with strong N2H+(1-0), HCO+(1-0), HCN(1-0), and HNC(1-0) emission from the Millimetre Astronomy Legacy Team 90 GHz survey. We obtained Herschel data for all 90 sources and NRAO VLA Sky Survey data for 51 of them. We convolved and regridded all images to the same resolution and pixel size and derived the temperature, H2 column density, molecules' abundances and abundance, and ratios of each pixel. Our analysis yields three main conclusions. First, the abundances of N2H+, HCO+, HCN, and HNC increase when the column density decreases and the temperature increases, with spatial variations in their abundances dominated by changes in the H2 column density. Second, the abundance ratios between N2H+, HCO+, HCN, and HNC also display systemic variations as a function of the column density due to the chemical properties of these molecules. Third, the sources associated with the 20cm continuum emission can be classified into four types based on the behavior of the abundances of the four molecules considered here as a function of this emission. The variations of the first three types could also be attributed to the variation of the H2 column density.</description><source format="bibcode">2019ApJS..243...13L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/243/13</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/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/291/943">J/A+A/291/943 : Protostellar cores (Ossenkopf+, 1994)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/124/205">J/A+AS/124/205 : W3 star-forming region 345 GHz survey (Helmich+ 1997)</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/ApJ/756/60">J/ApJ/756/60 : A 3mm line survey in 37 IR dark clouds (Sanhueza+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/777/157">J/ApJ/777/157 : 90GHz obs. of high-mass star-forming regions (Hoq+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/563/A97">J/A+A/563/A97 : IRAM 30m reduced spectra of 59 sources (Gerner+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/568/A41">J/A+A/568/A41 : ATLASGAL Compact Source Catalog: 280&lt;l&lt;60 (Urquhart+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/ApSS/361.191">J/other/ApSS/361.191 : High-mass star forming clumps from MALT90 (Zhang+, 2016)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/243/13</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/243/13</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/243/13</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/243/13</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/243/13</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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