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<ri:Resource created="2021-04-19T08:24:34Z" 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>Astrochemical study along M83 circumnuclear ring</title><shortName>J/ApJ/884/100</shortName><identifier>ivo://CDS.VizieR/J/ApJ/884/100</identifier><altIdentifier>doi:10.26093/cds/vizier.18840100</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Harada N.</name></creator><creator><name>Sakamoto K.</name></creator><creator><name>Martin S.</name></creator><creator><name>Watanabe Y.</name></creator><creator><name>Aladro R.</name></creator><creator><name>Riquelme D.,Hirota A.</name></creator><date role="Updated">2021-07-05T11:14:47Z</date><date role="Created">2021-04-19T08:24:34Z</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-physics</subject><subject>interstellar-medium</subject><subject>radio-astronomy</subject><subject>galaxies</subject><description>We report an astrochemical study on the evolution of interstellar molecular clouds and consequent star formation in the center of the barred spiral galaxy M83. We used the Atacama Large Millimeter/submillimeter Array (ALMA) to image molecular species indicative of shocks (SiO and CH_3_OH), dense cores (N_2_H^+^), and photodissociation regions (CN and CCH), as well as a radio recombination line (H41{alpha}) tracing active star-forming regions. M83 has a circumnuclear gas ring that is joined at two intersections by gas streams from the leading- edge gas lanes on the bar. We found elevated abundances of the shock and dense-core tracers in one of the orbit-intersecting areas, and found peaks of CN and H41{alpha} downstream. In the other orbit-intersection area, we found a similar enhancement of the shock tracers, but less variation of other tracers, and no sign of active star formation in the stream. We propose that the observed chemical variation or lack of it is due to the presence or absence of collision-induced evolution of molecular clouds and induced star formation. This work presents the clearest case of the chemical evolution in the circumnuclear rings of barred galaxies thanks to the ALMA resolution and sensitivity.</description><source format="bibcode">2019ApJ...884..100H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/884/100</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/361/1079">J/A+A/361/1079 : HNCO in massive galactic dense cores (Zinchenko, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/122/3046">J/AJ/122/3046 : HST photometry of star clusters in NGC 5236 (Harris+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/455/971">J/A+A/455/971 : Organic molecules in the Gal. center (Requena-Torres+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/174/337">J/ApJS/174/337 : Star formation in nuclear rings (Mazzuca+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/703/517">J/ApJ/703/517 : The Spitzer Local Volume Legacy: IR photometry (Dale+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/699/1092">J/ApJ/699/1092 : Giant molecular clouds (SRBY) (Heyer+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/421/2786">J/MNRAS/421/2786 : Modelling of shock waves mol. line emission (Flower+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/549/A39">J/A+A/549/A39 : A 3mm molecular line survey of NGC1068 (Aladro+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/563/L6">J/A+A/563/L6 : CIG 638 CCH, HCN. 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