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<ri:Resource created="2014-03-21T14:25:57Z" 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>Barium abundances in Cepheids</title><shortName>J/MNRAS/428/3252</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/428/3252</identifier><altIdentifier>doi:10.26093/cds/vizier.74283252</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Andrievsky S.M.</name></creator><creator><name>Lepine J.R.D.</name></creator><creator><name>Korotin S.A.</name></creator><creator><name>Luck R.E.</name></creator><creator><name>Kovtyukh V.V.,Maciel W.J.</name></creator><date role="Updated">2024-07-20T20:13:31Z</date><date role="Created">2014-03-21T14:25:57Z</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>We derived the barium atmospheric abundances for a large sample of Cepheids, comprising 270 stars. The sample covers a large range of Galactocentric distances, from about 4 to 15kpc, so it is appropriate to investigate the existence of radial barium abundance gradients in the Galactic disc. In fact, this is the first time that such a comprehensive analysis of the distribution of barium abundances in the Galactic disc has been carried out. As a result, we conclude that the Ba abundance distribution can be characterized by a zero gradient. This result is compared with derived gradients for other elements, and some reasons are briefly discussed for the independence of the barium abundances from Galactocentric distances.</description><source format="bibcode">2013MNRAS.428.3252A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/428/3252</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/381/32">J/A+A/381/32 : Galactic Cepheid abundances (Andrievsky+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/143/211">J/A+AS/143/211 : Galactic Cepheids BVRI photometry (Berdnikov+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/404/423">J/A+A/404/423 : BVI photometry of Galactic Cepheids (Tammann+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/534/A94">J/A+A/534/A94 : Milky Way Cepheids radial velocities (Storm+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/51">J/AJ/142/51 : Galactic Cepheids abundance variations (Luck+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/61/285">J/AcA/61/285 : VI light curves of Galactic Bulge Cepheids (Soszynski+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/193/12">J/ApJS/193/12 : JHK photometry of Northern Galactic Cepheids (Monson+, 2011)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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