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<ri:Resource created="2013-02-04T11:05:40Z" 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>Oxygen abundances and properties of galaxies</title><shortName>J/A+A/550/A115</shortName><identifier>ivo://CDS.VizieR/J/A+A/550/A115</identifier><altIdentifier>doi:10.26093/cds/vizier.35500115</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hughes T.M.</name></creator><creator><name>Cortese L.</name></creator><creator><name>Boselli A.</name></creator><creator><name>Gavazzi G.</name></creator><creator><name>Davies J.I.</name></creator><date role="Updated">2017-10-11T05:13:52Z</date><date role="Created">2013-02-04T11:05:40Z</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>galaxies</subject><subject>chemical-abundances</subject><description>We investigate the relationship between stellar mass, metallicity and gas content for a magnitude- and volume-limited sample of 260 nearby late-type galaxies in different environments, from isolated galaxies to Virgo cluster members. We derive oxygen abundance estimates using new integrated, drift scan optical spectroscopy and the base metallicity calibrations of Kewley &amp; Ellison (2008ApJ...681.1183K). Combining these measurements with ultraviolet to near- infrared photometry and HI 21cm line observations, we examine the relations between stellar mass, metallicity, gas mass fraction and star formation rate. We find that, at fixed stellar mass, galaxies with lower gas fractions typically also possess higher oxygen abundances. We also observe a relationship between gas fraction and metal content, whereby gas-poor galaxies are typically more metal-rich, and demonstrate that the removal of gas from the outskirts of spirals may increase the observed average metallicity by ~0.1dex. Although some cluster galaxies are gas-deficient objects, statistically the stellar-mass metallicity relation is nearly invariant to the environment, in agreement with recent studies. These results indicate that internal evolutionary processes, rather than environmental effects, play a key role in shaping the stellar mass - metallicity relation. 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Global oxygen abundance following Kewley &amp; Dopita, 2002ApJS..142...35K (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>O3N2</name><description>? Global oxygen abundance following Pettini &amp; Pagel, 2004MNRAS.348L..59P (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>N2</name><description>? Global oxygen abundance following Pettini &amp; Pagel, 2004MNRAS.348L..59P (1)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>M91c</name><description>? Global oxygen abundance following McGaugh, 1991ApJ...380..140M (1) (2)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Z94c</name><description>? 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Mean oxygen abundance, 12+log(O/H)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Nc</name><description>? Number of calibrations averaged</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Name</name><description>Galaxy name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>M</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>HRS</name><description>? Herschel Reference Survey number (Boselli et al. 2010, Cat. 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