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<ri:Resource created="2025-11-13T09:13:46Z" status="active" updated="2026-08-03T06:59:01Z" 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>Chromospherically active stars</title><shortName>J/A+A/703/A128</shortName><identifier>ivo://CDS.VizieR/J/A+A/703/A128</identifier><altIdentifier>doi:10.26093/cds/vizier/bc-nz/lbci</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bale B.</name></creator><creator><name>Tautvaisiene G.</name></creator><creator><name>Minkeviciute R.</name></creator><creator><name>Drazdauskas A.</name></creator><creator><name>Mikolaitis S.,Stonkute E.</name></creator><creator><name>Ambrosch M.</name></creator><date role="Updated">2026-08-03T06:59:01Z</date><date role="Created">2025-11-13T09:13:46Z</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>magnetic-fields</subject><subject>chemical-abundances</subject><description>We carried out a detailed investigation of Lthium and CNO abundances, including carbon isotope ratios, in RS CVn stars to assess the role of magnetic activity in the mixing of stellar atmospheres. High-resolution spectra were observed at the Moletai Astronomical Observatory to determine the lithium abundances by spectral synthesis of the 6707{AA} line and the CNO abundances using the C2 band heads at 5135 and 5635.5{AA}, CN bands at 6470-6490{AA} and 7980-8005{AA}, and the [O I] line at 6300{AA}. By fitting the ^13^CN band at 8004.7{AA}, we determined the carbon isotope ratios. We determined the main atmospheric parameters and investigated the chemical composition for 32 RS CVn stars. Lithium NLTE abundances were determined for 13 additional stars using archival spectra. We found that iota Gem and HD 179094 have carbon isotope ratios already affected by extra-mixing, even though being in the evolutionary stage below the red giant branch luminosity bump. About half of the low-mass giants, for which the lithium abundance was determined, follow the first dredge-up predictions; however, other stars have Li abundances reduced as predicted by the thermohaline-induced mixing. The intermediate-mass stars have Li abundances reduced as predicted by the rotation-induced mixing. We found that in low-mass chromospherically active RS CVn stars extra mixing of lithium along with carbon isotopes may begin earlier than in normal giants. The Li-rich RS CVn giant V* OP And has quite large C/N and carbon isotope ratios, and raises questions about the origin of its lithium enhancement.</description><source format="bibcode">2025A&amp;A...703A.128B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/703/A128</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></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/703/A128</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/703/A128</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/703/A128</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/703/A128</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/703/A128</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/703/A128</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/703/A128/tablea1 (Atmospheric parameters)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/703/A128/tablea1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/703/A128/tablea1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/703/A128/tablea1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>1.3339217</ra><dec>-5.70762</dec><sr>0.005555555555555556</sr></testQuery></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/A+A/703/A128/tablea2 (Lithium abundances)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/703/A128/tablea2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/703/A128/tablea2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/703/A128/tablea2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>1.3339217</ra><dec>-5.70762</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/1495 2839 2927 3579 4559 4772 5024 5028 5670 5676 6203 6219 6241 7451 8378 8667 8844-8845 8937 9541 10241 10407 10490 11764 12143 12155 12962 13462 13778 14020 14596 14630 15165 15409 17368 17989 18417 20102 22909 26302 27088 28252 29923 30431 32743</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/703/A128?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/A+A/703/A128/tablea1</name><description>Atmospheric parameters</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Number of CN lines</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>[O/H]</name><description>? Oxygen abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_[O/H]</name><description>Uncertainity in oxygen abundance</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>o_O</name><description>Number of oxygen lines</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[Mg/H]</name><description>Magnesium abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Mg/H]</name><description>Uncertainity in magnesium abundance</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>o_Mg</name><description>Number of magnesium lines</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>12C/13C</name><description>? 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>ID</name><description>Tycho-2 catalogue identification</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>Res</name><description>Spectral resolution</description><ucd>spect.resolution</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>A(Li)LTE</name><description>? Lithium abundance in LTE</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>A(Li)NLTE</name><description>? Lithium abundance in NLTE</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_A(Li)</name><description>? 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