J/A+A/564/A119ivo://CDS.VizieR/J/A+A/564/A119doi:10.26093/cds/vizier.35640119CDSMorel T.Miglio A.Lagarde N.Montalban J.Rainer M.Poretti E.,Eggenberger P.Hekker S.Kallinger T.Mosser B.Valentini M.,Carrier F.Hareter M.Mantegazza L.2018-01-04T08:22:33Z2014-04-16T09:15:19ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgiant-starsline-intensitieschemical-abundancesA precise characterisation of the red giants in the seismology fields of the CoRoT satellite is a prerequisite for further in-depth seismic modelling. High-resolution FEROS and HARPS spectra were obtained as part of the ground-based follow-up campaigns for 19 targets holding great asteroseismic potential. These data are used to accurately estimate in a self-consistent manner their fundamental parameters and the abundances of 16 chemical species. Some powerful probes of mixing are investigated (the Li and CNO abundances, as well as the carbon isotopic ratio in a few cases). The information provided by the spectroscopic and seismic data is combined to provide more accurate physical parameters and abundances. The stars in our sample follow the general trends between various abundance ratios and the metallicity observed in stars of the Galactic disk. After allowance is made for the chemical evolution of the interstellar medium, the observational signature of internal mixing phenomena is revealed through the detection at the stellar surface of the products of the CN and, in the case of the most massive stars, NeNa cycles. Together with the asteroseismic constraints, these data will pave the way for a detailed theoretical investigation of the physical processes responsible for the transport of chemical elements in evolved, low- and intermediate-mass stars.2014A&A...564A.119Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/564/A119CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/corot : CoRoT observation log Release 13 (CoRoT, 2009-2014)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/564/A119https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/564/A119http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/564/A119https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/564/A119https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/564/A119http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/564/A119GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/564/A119/table1 (Observations and basic target parameters)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/564/A119/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/564/A119/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/564/A119/table1?GETtext/xml+votable180.050000true90.20550532.91600690.0055555555555555566/8767 21462 21469 22047 22059 22440 22442 23564 24715 29558 30278 30294 30319 30339 30416 30447 30529 30953 31809 31812 31814 318323.322582951404819e-19 3.852589004194616e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/564/A119?format=asciiOpticaldefaultJ/A+A/564/A119/table1Observations and basic target parametersHR? HR (Bright Star) designationmeta.idintnullableHDHD identificationmeta.idintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHIP? Hipparcos identification (I/311)meta.idintnullableNameStar name (as in the other tables)meta.id;meta.maincharprimaryEWDisplay the 116 equivalent widthsmeta.ref.urlcharAbSimbad column added by the CDSmeta.ref.urlcharSpTMK spectral type (from Simbad)src.spTypecharVmagMagnitude in theV band (from Simbad)magphot.mag;em.opt.VfloatPlx? Parallaxmaspos.parallax.trigfloatnullablee_Plx? Mean error on Plxmasstat.error;pos.parallaxfloatnullablen_Plx[a] Parallax of NGC 6633 (van Leeuwen 2009A&A...497..209V)meta.notecharInstrInstrumentmeta.id;instrcharRResolving power ({lambda}/{Delta}{lambda})spect.resolutionintBroadInstrumental broadening ({AA})0.1nmspect.line.broadfloatNsp[1/181] Number of spectrameta.numberintS/NSignal/Noise at 5815{AA} (see associated flag)stat.snrintf_S/NFlag on S/N: b = mean S/N over 3600-9300{AA}, c = S/N at 5500{AA}meta.codecharSimbadSimbad column added by the CDSmeta.ref.urlchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainJ/A+A/564/A119/tablea2Equivalent width measurementsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namemeta.id;meta.maincharIonIon designationphys.atmol.ionStagecharlambdaLine wavelength {lambda}0.1nmem.wl;spect.linedoubleEW? Equivalent width0.1pmspect.line.eqWidthfloatnullableJ/A+A/564/A119/tablea3Line list and atomic datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIonIon designationphys.atmol.ionStagecharlambdaLine wavelength {lambda}0.1nmem.wl;spect.linedoubleLEPLower excitation potentialeVphys.atmol.excitation;stat.minfloatlog(gf)Oscillator strengthphys.atmol.oscStrengthfloatlog(C6)? Interaction constant for van der Waals interaction (1)arith.zpfloatnullableEgamma? Enhancement factor to the line width parameter (to the power 5/2)phys.atmol.dampingfloatnullableJ/A+A/564/A119/abundAbundance data for Mg, Al, Si, Ca, Sc, Ti, Cr, Co, Ni, and Ba (tablea4), mixing indicators (Li, C, N, O, Na and 12C/13C) (tablea5), and abundance ratios of C, N, and O (tablea6)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namemeta.id;meta.maincharMet[A/I] Method to derive logg (G1)meta.notechar[Mg/Fe]Abundance ratio [Mg/Fe]log(Sun)phys.abund;arith.ratiofloate_[Mg/Fe]Uncertainty on [Mg/Fe]log(Sun)stat.error;phys.abundfloat[Al/Fe]Abundance ratio [Al/Fe]log(Sun)phys.abund;arith.ratiofloate_[Al/Fe]Uncertainty on [Al/Fe]log(Sun)stat.error;phys.abundfloat[Si/Fe]Abundance ratio [Si/Fe]log(Sun)phys.abund;arith.ratiofloate_[Si/Fe]Uncertainty on [Si/Fe]log(Sun)stat.error;phys.abundfloat[Ca/Fe]Abundance ratio [Ca/Fe]log(Sun)phys.abund;arith.ratiofloate_[Ca/Fe]Uncertainty on [Ca/Fe]log(Sun)stat.error;phys.abundfloat[Sc/Fe]? Abundance ratio [Sc/Fe]log(Sun)phys.abund;arith.ratiofloatnullablee_[Sc/Fe]? Uncertainty on [Sc/Fe]log(Sun)stat.error;phys.abundfloatnullable[Ti/Fe]Abundance ratio [Ti/Fe]log(Sun)phys.abund;arith.ratiofloate_[Ti/Fe]Uncertainty on [Ti/Fe]log(Sun)stat.error;phys.abundfloat[Cr/Fe]Abundance ratio [Cr/Fe]log(Sun)phys.abund;arith.ratiofloate_[Cr/Fe]Uncertainty on [Cr/Fe]log(Sun)stat.error;phys.abundfloat[Co/Fe]Abundance ratio [Co/Fe]log(Sun)phys.abund;arith.ratiofloate_[Co/Fe]Uncertainty on [Co/Fe]log(Sun)stat.error;phys.abundfloat[Ni/Fe]Abundance ratio [Ni/Fe]log(Sun)phys.abund;arith.ratiofloate_[Ni/Fe]Uncertainty on [Ni/Fe]log(Sun)stat.error;phys.abundfloat[Ba/Fe]Abundance ratio [Ba/Fe]log(Sun)phys.abund;arith.ratiofloate_[Ba/Fe]Uncertainty on [Ba/Fe]log(Sun)stat.error;phys.abundfloat[Li/H]ELTE Abundance ratio [Li/H]log(Sun)phys.abund;arith.ratiofloate_[Li/H]E? Uncertainty on [Li/H]Elog(Sun)stat.error;phys.abundfloatnullable[Li/H]NNLTE Abundance ratio [Li/H] (2)log(Sun)phys.abund;arith.ratiofloate_[Li/H]N? Uncertainty on [Li/H]N (2)log(Sun)stat.error;phys.abundfloatnullablef_[Li/H][L/D] Flag for upper limit (L) or detection (D) of Lithiummeta.codechar[C/Fe]Abundance ratio [C/Fe]log(Sun)phys.abund;arith.ratiofloate_[C/Fe]Uncertainty on [C/Fe]log(Sun)stat.error;phys.abundfloat[C/Fe]cCorrected [C/Fe] abundance ratio (3)log(Sun)phys.abund;arith.ratiofloate_[C/Fe]cUncertainty on [C/Fe]c (3)log(Sun)stat.error;phys.abundfloat[N/Fe]Abundance ratio [N/Fe]log(Sun)phys.abund;arith.ratiofloate_[N/Fe]Uncertainty on [N/Fe]log(Sun)stat.error;phys.abundfloat[OI/Fe]Abundance ratio [OI 6300/Fe]log(Sun)phys.abund;arith.ratiofloate_[OI/Fe]Uncertainty on [OI/Fe]log(Sun)stat.error;phys.abundfloat[OI/Fe]cCorrected [OI 6300/Fe] abundance ratio (3)log(Sun)phys.abund;arith.ratiofloate_[OI/Fe]cUncertainty on [OI/Fe]c (3)log(Sun)stat.error;phys.abundfloat[Ot/Fe]? [O triplet/Fe] abundance ratiolog(Sun)phys.abund;arith.ratiofloatnullablee_[Ot/Fe]? Uncertainty on [Ott/Fe]log(Sun)stat.error;phys.abundfloatnullable[Na/Fe]Abundance ratio [Na/Fe]log(Sun)phys.abund;arith.ratiofloate_[Na/Fe]Uncertainty on [Na/Fe]log(Sun)stat.error;phys.abundfloat[Na/Fe]cCorrected [Na/Fe] abundance ratio (3)log(Sun)phys.abund;arith.ratiofloate_[Na/Fe]cUncertainty on [Na/Fe]c (3)log(Sun)stat.error;phys.abundfloat12C/13C? ^12^C/^13^C isotopic ratiophys.abundintnullablee_12C/13C? Uncertainty on 12C/13Cstat.errorintnullable[N/C]Abundance ratio [N/C]log(Sun)phys.abundfloate_[N/C]Uncertainty on [N/C]log(Sun)stat.error;phys.abundfloat[N/C]cCorrected [N/C] abundance ratio (4)log(Sun)phys.abundfloate_[N/C]cUncertainty on [N/C]c (4)log(Sun)stat.error;phys.abundfloat[N/O]Abundance ratio [N/O]log(Sun)phys.abundfloate_[N/O]Uncertainty on [N/O]log(Sun)stat.error;phys.abundfloat[N/O]cCorrected [N/O] abundance ratio (4)log(Sun)phys.abundfloate_[N/O]cUncertainty on [N/O]c (4)log(Sun)stat.error;phys.abundfloat[C/O]Abundance ratio [C/O]log(Sun)phys.abundfloate_[C/O]Uncertainty on [C/O]log(Sun)stat.error;phys.abundfloat[C/O]cCorrected [C/O] abundance ratio (4)log(Sun)phys.abundfloate_[C/O]cUncertainty on [C/O]c (4)log(Sun)stat.error;phys.abundfloat