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<ri:Resource created="2012-11-20T09:54:20Z" 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>Galactic Cepheids abundance variations</title><shortName>J/AJ/142/51</shortName><identifier>ivo://CDS.VizieR/J/AJ/142/51</identifier><altIdentifier>doi:10.26093/cds/vizier.51420051</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Luck R.E.</name></creator><creator><name>Andrievsky S.M.</name></creator><creator><name>Kovtyukh V.V.</name></creator><creator><name>Gieren W.</name></creator><creator><name>Graczyk D.</name></creator><date role="Updated">2017-06-19T07:57:19Z</date><date role="Created">2012-11-20T09:54:20Z</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>variable-stars</subject><subject>chemical-abundances</subject><description>This paper reports on the spectroscopic investigation of 101 Cepheids in the Carina region. These Cepheids extend previous samples by about 35% in number and increase the amount of the Galactic disk coverage especially in the direction of l~~270{deg}. The new Cepheids do not add much information to the radial gradient, but provide a substantial increase in azimuthal coverage. We find no azimuthal dependence in abundance over an 80{deg} angle from the Galactic center in an annulus of 1kpc depth centered on the Sun. A simple linear fit to the Cepheid data yields a gradient d[Fe/H]/dR_G_=-0.055+/-0.003dex/kpc which is somewhat shallower than found from our previous, smaller Cepheid sample.</description><source format="bibcode">2011AJ....142...51L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/142/51</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+A/392/491">J/A+A/392/491 : Galactic abundance gradient. III. (Andrievsky+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/381/32">J/A+A/381/32 : Galactic Cepheid abundances (Andrievsky+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/413/159">J/A+A/413/159 : Galactic abundance gradient. V. 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