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<ri:Resource created="2023-02-03T14:57:31Z" 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>Two new Galactic lithium-rich Cepheids</title><shortName>J/MNRAS/488/3211</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/488/3211</identifier><altIdentifier>doi:10.26093/cds/vizier.74883211</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kovtyukh V.</name></creator><creator><name>Lemasle B.</name></creator><creator><name>Kniazev A.</name></creator><creator><name>Berdnikov L.</name></creator><creator><name>Bono G.</name></creator><creator><name>Usenko I.,Grebel E.K.</name></creator><creator><name>Hajdu G.</name></creator><creator><name>Pastukhova E.</name></creator><date role="Updated">2024-08-20T20:12:10Z</date><date role="Created">2023-02-03T14:57:31Z</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>stellar-distance</subject><subject>effective-temperature</subject><subject>radial-velocity</subject><subject>chemical-abundances</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><description>We report the discovery of two new lithium-rich Cepheids in the Milky Way (A(Li)~2.9dex) among the targets of the MAGIC spectroscopic survey with the Southern African Large Telescope spectrographs. The 6707{AA} Li feature is usually not detectable in the atmosphere of Cepheids. Only three Cepheids (two in the Milky Way and one in the Large Magellanic Cloud) had been reported so far with high lithium abundances. We examine the possibility that the Li-rich Cepheids are evolving towards the red giant branch, crossing the instability strip for the first time, as well as other possible scenarios. The two stars are mixed-mode Cepheids pulsating simultaneously in the first and in the second overtone modes. 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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>Name</name><description>Cepheid name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>Type</name><description>Cepheid type</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>Mode</name><description>Pulsating modes</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>RG</name><description>Galactocentric distance</description><unit>kpc</unit><ucd>pos.distance;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>Distance</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>GLON</name><description>Galactic longitude (l)</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>Galactic latitude (b)</description><unit>deg</unit><ucd>pos.galactic.lat</ucd></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data. 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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>Name</name><description>Cepheid name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>[FeI/H]</name><description>FeI to hydrogen abundance ratio</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[FeI/H]</name><description>Error on [FeI/H]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>o_[FeI/H]</name><description>Number of lines used to obtain [FeI/H]</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[FeII/H]</name><description>FeII to hydrogen abundance ratio</description><ucd>phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[FeII/H]</name><description>Error on [FeII/H]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>o_[FeII/H]</name><description>Number of lines used to obtain [FeII/H]</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>A(Li)</name><description>Lithium abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_A(Li)</name><description>Error on A(Li)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>o_A(Li)</name><description>Number of lines used to obtain A(Li)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[C/H]</name><description>Carbon to hydrogen abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[C/H]</name><description>Error on [C/H]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>o_[C/H]</name><description>Number of lines used to obtain [C/H]</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[N/H]</name><description>Nitrogen to hydrogen abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[N/H]</name><description>Error on [N/H]</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>o_[N/H]</name><description>Number of lines used to obtain [N/H]</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>[O/H]</name><description>Oxygen to hydrogen abundance ratio</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[O/H]</name><description>? 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