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<ri:Resource created="2014-04-09T09:34:01Z" 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>HII regions in the Magellanic clouds from MCELS</title><shortName>J/ApJ/755/40</shortName><identifier>ivo://CDS.VizieR/J/ApJ/755/40</identifier><altIdentifier>doi:10.26093/cds/vizier.17550040</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pellegrini E.W.</name></creator><creator><name>Oey M.S.</name></creator><creator><name>Winkler P.F.</name></creator><creator><name>Points S.D.</name></creator><creator><name>Smith R.C.,Jaskot A.E.</name></creator><creator><name>Zastrow J.</name></creator><date role="Updated">2017-10-13T15:41:48Z</date><date role="Created">2014-04-09T09:34:01Z</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>h-ii-regions</subject><subject>magellanic-clouds</subject><description>We exploit ionization-parameter mapping (IPM) as a powerful tool to measure the optical depth of star-forming H II regions. Our simulations using the photoionization code CLOUDY and our new, SURFBRIGHT surface-brightness simulator demonstrate that this technique can directly diagnose most density-bounded, optically thin nebulae using spatially resolved emission-line data. We apply this method to the Large and Small Magellanic Clouds (LMC and SMC), using the data from the Magellanic Clouds Emission Line Survey. We generate new H II region catalogs based on photoionization criteria set by the observed ionization structure in the [S II]/[O III] ratio and H{alpha} surface brightness. The luminosity functions from these catalogs generally agree with those from H{alpha}-only surveys. We then use IPM to crudely classify all the nebulae into optically thick versus optically thin categories, yielding fundamental new insights into Lyman-continuum (LyC) radiation transfer.</description><source format="bibcode">2012ApJ...755...40P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/755/40</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/VII/232">VII/232 : Nebulae in the Magellanic Clouds (Davies+ 1976)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/509/A11">J/A+A/509/A11 : SMC clusters H{alpha} emission-line objects (Martayan+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/184/1">J/ApJS/184/1 : Molecular clouds in the LMC by NANTEN. 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