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<ri:Resource created="2010-12-01T15:03:56Z" 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 Ba stars</title><shortName>J/A+A/525/A63</shortName><identifier>ivo://CDS.VizieR/J/A+A/525/A63</identifier><altIdentifier>doi:10.26093/cds/vizier.35250063</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Allen D.M.</name></creator><creator><name>Porto de Mello G.F.</name></creator><date role="Updated">2017-06-26T11:50:05Z</date><date role="Created">2010-12-01T15:03:56Z</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>peculiar-variable-stars</subject><subject>chemical-abundances</subject><description>We present abundances of Mn, Cu, Zn, and various light and heavy elements for a sample of barium and normal giant stars, and present correlations between abundances contributed to different degrees by the weak-s, main-s, and r-processes of neutron capture, between Fe-peak elements and heavy elements. All spectra for the sample stars were obtained with the 1.52m telescope at ESO, La Silla, using the Fiber Fed Extended Range Optical Spectrograph (FEROS). FEROS spectra have a constant resolving power of R=48000 from 3600{AA} to 9200{AA}. The stellar sample targeted in our study includes eight mild and classical barium stars and six normal giants, with a spectral S/N ratio ranging from 200 to 450 in the visible range.</description><source format="bibcode">2011A&amp;A...525A..63A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/525/A63</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/II/192">II/192 : UBV Photometry of Barium Stars (Watanabe+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/81">V/81 : Taxonomy of Barium Stars (Lu 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/319/881">J/A+A/319/881 : Ba II strength of barium stars (Gomez+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/321/L9">J/A+A/321/L9 : Barium stars in the HR diagram (Bergeat+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/326/722">J/A+A/326/722 : HIPPARCOS Ba stars (Mennessier+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/372/245">J/A+A/372/245 : Infrared properties of barium stars (Chen+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/79/909">J/AZh/79/909 : Chemical abundances in barium stars (Boyarchuk+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/80/704">J/AZh/80/704 : Studies of classical barium stars (Antipova+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/454/895">J/A+A/454/895 : Abundances of 26 barium stars. I. (Allen+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/454/917">J/A+A/454/917 : Abundances of 26 barium stars. II. 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