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<ri:Resource created="2009-06-14T05:12:49Z" 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>VLT-FLAMES survey of massive stars</title><shortName>J/A+A/496/841</shortName><identifier>ivo://CDS.VizieR/J/A+A/496/841</identifier><altIdentifier>doi:10.26093/cds/vizier.34960841</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hunter I.</name></creator><creator><name>Brott I.</name></creator><creator><name>Langer N.</name></creator><creator><name>Lennon D.J.</name></creator><creator><name>Dufton P.L.</name></creator><creator><name>Howarth I.D.,Ryans R.S.I.</name></creator><creator><name>Trundle C.</name></creator><creator><name>Evans C.J.</name></creator><creator><name>De Koter A.</name></creator><creator><name>Smartt S.J.</name></creator><date role="Updated">2017-12-18T07:57:11Z</date><date role="Created">2009-06-14T05:12:49Z</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>open-star-clusters</subject><subject>early-type-stars</subject><subject>chemical-abundances</subject><description>We have previously analysed the spectra of 135 early B-type stars in the Large Magellanic Cloud (LMC) and found several groups of stars that have chemical compositions that conflict with the theory of rotational mixing. Here we extend this study to Galactic and Small Magellanic Cloud (SMC) metallicities. We provide chemical compositions for ~50 Galactic and ~100 SMC early B-type stars and compare these to the LMC results. These samples cover a range of projected rotational velocities up to ~300km/s and hence are well suited to testing rotational mixing models. The surface nitrogen abundances are utilised as a probe of the mixing process since nitrogen is synthesized in the core of the stars and mixed to the surface.</description><source format="bibcode">2009A&amp;A...496..841H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/496/841</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/437/467">J/A+A/437/467 : VLT-FLAMES survey of massive stars (Evans+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/456/623">J/A+A/456/623 : VLT-FLAMES survey of massive stars (Evans+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/457/265">J/A+A/457/265 : VLT-FLAMES survey of massive stars (Dufton+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/466/277">J/A+A/466/277 : VLT-FLAMES survey of massive stars (Hunter+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/471/625">J/A+A/471/625 : VLT-FLAMES survey of massive stars (Trundle+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/479/541">J/A+A/479/541 : VLT-FLAMES survey of massive stars (Hunter+, 2008)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/496/841</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/496/841</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/496/841</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/496/841</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/496/841</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/496/841</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/A+A/496/841/table2 (Atmospheric parameters, projected rotational velocities and chemical compositions of the sample)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/496/841/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/496/841/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/496/841/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>274.7445464</ra><dec>-13.9912331</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/29463 29506 33112 33126 33295 33317 33328 38018-38019 38024 43033 43036</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/496/841?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/496/841/table2</name><description>Atmospheric parameters, projected rotational velocities and chemical compositions of the sample</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Number of lines observed for Si abundance</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/A+A/496/841/table1</name><description>Equivalent width measurements and derived abundances for the metal lines observed in the spectra of our sample stars</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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