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<ri:Resource created="2013-01-18T09:29:54Z" 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>NGC253 near-infrared H_2_ emission</title><shortName>J/A+A/550/A12</shortName><identifier>ivo://CDS.VizieR/J/A+A/550/A12</identifier><altIdentifier>doi:10.26093/cds/vizier.35500012</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rosenberg M.J.F.</name></creator><creator><name>van der Werf P.P.</name></creator><creator><name>Israel F.P.</name></creator><date role="Updated">2017-06-30T05:48:31Z</date><date role="Created">2013-01-18T09:29:54Z</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>seyfert-galaxies</subject><subject>molecular-clouds</subject><subject>infrared-photometry</subject><description>Because of its large angular size and proximity to the Milky Way, NGC 253, an archetypal starburst galaxy, provides an excellent laboratory to study the intricacies of this intense episode of star formation. We aim to characterize the excitation mechanisms driving the emission in NGC 253. 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