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<ri:Resource created="2015-04-22T08:03:51Z" 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>M17-SW datacubes in C and CO lines</title><shortName>J/A+A/575/A9</shortName><identifier>ivo://CDS.VizieR/J/A+A/575/A9</identifier><altIdentifier>doi:10.26093/cds/vizier.35750009</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Perez-Beaupuits J.P.</name></creator><creator><name>Stutzki J.</name></creator><creator><name>Ossenkopf V.</name></creator><creator><name>Spaans M.</name></creator><creator><name>Gusten R.,Wiesemeyer H.</name></creator><date role="Updated">2015-07-28T10:46:35Z</date><date role="Created">2015-04-22T08:03:51Z</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>co-line-emission</subject><subject>h-ii-regions</subject><subject>nebulae</subject><subject>radio-astronomy</subject><subject>millimeter-astronomy</subject><subject>submillimeter-astronomy</subject><subject>molecular-clouds</subject><subject>spectroscopy</subject><description>We probe the column densities and masses traced by the ionized [CII] and neutral [CI] atomic carbon with spectrally resolved maps, and compare them to the diffuse and dense molecular gas traced by [CI] and low-J CO lines toward the star-forming region M17 SW. We mapped a 4.1pcx4.7pc region in the [CI] 609{mu}m line using the APEX telescope, as well as the CO isotopologues with the IRAM 30m telescope. Data are analyzed based on velocity channel maps that are 1km/s wide. We correlate their spatial distribution with that of the [CII] map obtained with SOFIA/GREAT. 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