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<ri:Resource created="1999-04-12T17:12:12Z" 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>H II regions in spiral galaxies</title><shortName>J/AJ/116/2805</shortName><identifier>ivo://CDS.VizieR/J/AJ/116/2805</identifier><altIdentifier>doi:10.26093/cds/vizier.51162805</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Van Zee L.</name></creator><creator><name>Salzer J.J.</name></creator><creator><name>Haynes M.P.</name></creator><creator><name>O'Donoghue A.A.</name></creator><creator><name>Balonek T.J.</name></creator><date role="Updated">2023-04-06T16:50:31Z</date><date role="Created">1999-04-12T17:12:12Z</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>galaxies</subject><subject>visible-astronomy</subject><subject>chemical-abundances</subject><description>We present the results of low-dispersion optical spectroscopy of 186 HII regions spanning a range of radius in 13 spiral galaxies. Abundances for several elements (oxygen, nitrogen, neon, sulfur, and argon) were determined for 185 of the HII regions. As expected, low metallicities were found for the outlying HII regions of these spiral galaxies. Radial abundance gradients were derived for the 11 primary galaxies; similar to results for other spiral galaxies, the derived abundance gradients are typically -0.04 to -0.07dex/kpc.</description><source format="bibcode">1998AJ....116.2805V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/116/2805</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/118">VII/118 : NGC 2000.0 (Sky Publishing, ed. 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Radius</description><unit>arcsec</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/AJ/116/2805/table2</name><description>Spectroscopy observing log</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NGC</name><description>NGC (Cat. &lt;VII/118&gt;) galaxy designation</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>NHII</name><description>Number of HII regions</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>12+log(O/H)</name><description>Central 12+log(O/H) abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_12+log(O/H)</name><description>rms uncertainty on 12+log(O/H)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gradient1</name><description>Gradient in dex/r_25_</description><ucd>arith.grad;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Gradient1</name><description>rms uncertainty on Gradient1</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gradient2</name><description>Gradient in dex/r_d_</description><ucd>arith.grad;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Gradient2</name><description>rms uncertainty on Gradient2</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Gradient3</name><description>Gradient in dex/kpc</description><ucd>arith.grad;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Gradient3</name><description>rms uncertainty on Gradient3</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>