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<ri:Resource created="2021-07-22T08:59:38Z" 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>Li abundance and mixing in giant stars</title><shortName>J/A+A/651/A84</shortName><identifier>ivo://CDS.VizieR/J/A+A/651/A84</identifier><altIdentifier>doi:10.26093/cds/vizier.36510084</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Magrini L.</name></creator><creator><name>Lagarde N.</name></creator><creator><name>Charbonnel C.</name></creator><creator><name>Franciosini E.</name></creator><creator><name>Randich S.,Smiljanic R.</name></creator><creator><name>Casali G.</name></creator><creator><name>Viscasillas Vazquez C.</name></creator><creator><name>Spina L.</name></creator><creator><name>Biazzo K.,Pasquini L.</name></creator><creator><name>Bragaglia A.</name></creator><creator><name>Van der Swaelmen M.</name></creator><creator><name>Tautvaisiene G.</name></creator><creator><name>Inno L.,Sanna N.</name></creator><creator><name>Prisinzano L.</name></creator><creator><name>Degl'Innocenti S.</name></creator><creator><name>Prada Moroni P.,Roccatagliata V.</name></creator><creator><name>Tognelli E.</name></creator><creator><name>Monaco L.</name></creator><creator><name>de Laverny P.</name></creator><creator><name>Delgado-Mena E.,Baratella M.</name></creator><creator><name>D'Orazi V.</name></creator><creator><name>Vallenari A.</name></creator><creator><name>Gonneau A.</name></creator><creator><name>Worley C.,Jimenez-Esteban F.</name></creator><creator><name>Jofre P.</name></creator><creator><name>Bensby T.</name></creator><creator><name>Francois P.</name></creator><creator><name>Guiglion G.</name></creator><creator><name>Bayo A.,Jeries R.D.</name></creator><creator><name>Binks A.S.</name></creator><creator><name>Gilmore G.</name></creator><creator><name>Damiani F.</name></creator><creator><name>Korn A.</name></creator><creator><name>Pancino E.,Sacco G.G.</name></creator><creator><name>Hourihane A.</name></creator><creator><name>Morbidelli L.</name></creator><creator><name>Zaggia S.</name></creator><date role="Updated">2023-02-04T18:38:24Z</date><date role="Created">2021-07-22T08:59:38Z</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>milky-way-galaxy</subject><subject>open-star-clusters</subject><subject>giant-stars</subject><subject>chemical-abundances</subject><description>We aim to constrain the mixing processes in low-mass stars by investigating the behaviour of the Li surface abundance after the main sequence. We take advantage of the data from the sixth internal data release of Gaia-ESO, idr6, and from the Gaia Early Data Release 3, EDR3. We selected a sample of main-sequence, sub-giant, and giant stars in which the Li abundance is measured by the Gaia-ESO survey. These stars belong to 57 open clusters with ages from 130Myr to about 7Gyr and to Milky Way fields, covering a range in [Fe/H] between -1.0 and +0.5dex, with few stars between -1.0 and -2.5dex. We studied the behaviour of the Li abundances as a function of stellar parameters. We inferred the masses of giant stars in clusters from the main-sequence turn-off masses, and for field stars through comparison with stellar evolution models using a maximum likelihood technique. We compared the observed Li behaviour in field giant stars and in giant stars belonging to individual clusters with the predictions of a set of classical models and of models with mixing induced by rotation and thermohaline instability. The comparison with stellar evolution models confirms that classical models cannot reproduce the observed lithium abundances in the metallicity and mass regimes covered by the data. The models that include the effects of both rotation-induced mixing and thermohaline instability account for the Li abundance trends observed in our sample in all metallicity and mass ranges. The differences between the results of the classical models and of the rotation models largely differ (up to~2 dex), making lithium the best element with which to constrain stellar mixing processes in low-mass stars. We discuss the nature of a sample of Li-rich stars. We demonstrate that the evolution of the surface abundance of Li in giant stars is a powerful tool for constraining theoretical stellar evolution models, allowing us to distinguish the effect of different mixing processes. For stars with well-determined masses, we find a better agreement of observed surface abundances and models with rotation-induced and thermohaline mixing. Rotation effects dominate during the main sequence and the first phases of the post-main-sequence evolution, and the thermohaline induced mixing after the bump in the luminosity function.</description><source format="bibcode">2021A&amp;A...651A..84M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/651/A84</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/566/A50">J/A+A/566/A50 : Classification of stellar spectra 644-681nm (Damiani+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/640/A1">J/A+A/640/A1 : Portrait Galactic disc 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(2020A&amp;A...640A...1C, Cat. J/A+A/640/A1)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Rgc</name><description>Galactocentric distance from Cantat-Gaudin et al. (2020A&amp;A...640A...1C, Cat. J/A+A/640/A1)</description><unit>kpc</unit><ucd>pos.distance;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rv</name><description>Mean cluster radial velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_rv</name><description>? Error on the Mean radial velocity</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Fe/H]m</name><description>Mean cluster metallicity in the solar scale</description><ucd>instr.scale;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Fe/H]m</name><description>? Error on the Mean cluster metallicity</description><ucd>stat.error;phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MMSTO</name><description>Main Sequence Turn Off (MSTO) mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>AgeIso</name><description>Age of the Isochrone used to compute the MSTO</description><unit>Gyr</unit><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ZIso</name><description>Metallicity (by mass) of the Isochrone used to compute the MSTO</description><ucd>phys.abund.Z</ucd><dataType xsi:type="vs:VOTableType">float</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/651/A84/tablea2</name><description>Cluster member stars</description><column><name>l_Li1</name><description>Upper limit flag for Li1</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Li1</name><description>Lithium abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Li1</name><description>? Error on Lithium abundance</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Gamma</name><description>? Gravity index defined in Damiani et al. (2014A&amp;A...566A..50D, Cat. J/A+A/566/A50)</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Gamma</name><description>? Error on the Gravity index defined in Damiani et al. (2014A&amp;A...566A..50D, Cat. J/A+A/566/A50)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logL</name><description>? Stellar Luminosity in log</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logL</name><description>? Error on the stellar Luminosity in log</description><unit>log(solLum)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MMSTO</name><description>Main Sequence Turn Off mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA</name><description>Positions from CName (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CName</name><description>Gaia ESO ID (HHMMSSss+DDMMSSs)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>GESField</name><description>Gaia ESO Field</description><ucd>obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="10*">char</dataType></column><column><name>Teff</name><description>Effective Temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Teff</name><description>Error on the Effective Temperature</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>Surface gravity</description><unit>log(cm.s**-1)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logg</name><description>Error on Surface gravity</description><unit>log(cm.s**-1)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Fe/H]</name><description>Iron abundance on the solar scale</description><ucd>instr.scale</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Fe/H]</name><description>Error on Iron abundance on the solar scale</description><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>_DE</name><description>Positions from CName (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/A+A/651/A84/tablea3</name><description>Field stars</description><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CName</name><description>Gaia ESO ID (HHMMSSss+DDMMSSs)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>GESField</name><description>Gaia ESO Field</description><ucd>obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>Teff</name><description>Effective Temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Teff</name><description>Error on the Effective Temperature</description><unit>K</unit><ucd>stat.error;phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>? Surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logg</name><description>? Error on Surface gravity</description><unit>log(cm.s**-2)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>[Fe/H]</name><description>Iron abundance on the solar scale</description><unit>log(Sun)</unit><ucd>instr.scale</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Fe/H]</name><description>Error on Iron abundance on the solar scale</description><unit>log(Sun)</unit><ucd>stat.error;phys.abund.Fe</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>l_Li1</name><description>Upper limit flag on Li1</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Li1</name><description>Lithium abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Li1</name><description>? Error on Lithium abundance</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Gamma</name><description>? Gravity index defined in Damiani et al. (2014A&amp;A...566A..50D, Cat. J/A+A/566/A50)</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Gamma</name><description>? Error on the Gravity index defined in Damiani et al. (2014A&amp;A...566A..50D, Cat. J/A+A/566/A50)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>logL</name><description>Stellar Luminosity in log</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_logL</name><description>Error on the stellar Luminosity in log</description><unit>log(solLum)</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mass</name><description>Mass</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_Mass</name><description>Error (positive) on the mass</description><unit>solMass</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Mass</name><description>Error (negative) on the mass</description><unit>solMass</unit><ucd>stat.error;phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>_RA</name><description>Positions from CName (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from CName (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>