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<ri:Resource created="2013-08-12T13:50:29Z" 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>Abundances in HII regions</title><shortName>J/MNRAS/424/2316</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/424/2316</identifier><altIdentifier>doi:10.26093/cds/vizier.74242316</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pilyugin L.S.</name></creator><creator><name>Grebel E.K.</name></creator><creator><name>Mattsson L.</name></creator><date role="Updated">2024-07-18T20:18:49Z</date><date role="Created">2013-08-12T13:50:29Z</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>chemical-abundances</subject><description>We suggest a new way of determining abundances and electron temperatures in HII regions from strong emission lines. Our approach is based on the standard assumption that HII regions with similar intensities of strong emission lines have similar physical properties and abundances. A 'counterpart' for a studied HII region may be chosen among HII regions with well-measured abundances (reference HII regions) by comparison of carefully chosen combinations of strong-line intensities. Then the abundances in the investigated HII region can be assumed to be the same as those in its counterpart. In other words, we suggest to determine the abundances in HII regions 'by precedent'. To get more reliable abundances for the considered HII region, a number of reference HII regions are selected and then the abundances in the target HII region are estimated through extrapolation/interpolation. We will refer to this method of abundance determination as the counterpart method or, for brevity, the C method. We define a sample of reference HII regions and verify the validity of the C method. We find that this method produces reliable abundances. Finally, the C method is used to obtain the radial abundance distributions in the extended discs of the spiral galaxies M83, NGC 4625 and NGC 628.</description><source format="bibcode">2012MNRAS.424.2316P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/424/2316</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+AS/91/285">J/A+AS/91/285 : HII galaxies spectrophotometric catalogue (Terlevich+, 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/116/2805">J/AJ/116/2805 : HII regions in spiral galaxies (Van Zee+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/121/169">J/AJ/121/169 : Imaging and spectroscopy of Tol 1214-277 (Fricke+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/421/539">J/A+A/421/539 : VLT spectroscopy of Tol 1214-277 + Tol 65 (Izotov+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/602/200">J/ApJ/602/200 : HII regions abundances in blue compact galaxies (Izotov+ 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/602/200">J/ApJ/602/200 : HII regions abundances in blue compact galaxies (Izotov+ 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/441/981">J/A+A/441/981 : HII regions in 5 spiral galaxies (Bresolin+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/636/214">J/ApJ/636/214 : HII regions in dwarf irregular galaxies (van Zee+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/656/168">J/ApJ/656/168 : Spectrophotometry in NGC 5253 (Lopez-Sanchez+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/464/885">J/A+A/464/885 : Abundances in 53 HII regions (Guseva+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/476/89">J/A+A/476/89 : HII galaxies narrow-band Hbeta images (Lagos+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/662/15">J/ApJ/662/15 : Abundances in extragalactic HII regions (Izotov+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/700/654">J/ApJ/700/654 : Keck spectroscopy of extragalactic HII regions (Esteban+ 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/521/A3">J/A+A/521/A3 : Abundances in HII regions and PNe of M81 (Stanghellini+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/529/A149">J/A+A/529/A149 : HII regions in low-metallicity galaxies (Guseva+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/533/A25">J/A+A/533/A25 : 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