J/A+A/468/663ivo://CDS.VizieR/J/A+A/468/663doi:10.26093/cds/vizier.34680663CDSTakeda Y.Kawanomoto S.Honda S.Ando H.Sakurai T.2017-06-13T11:08:07Z2007-08-15T08:44:22ZCDS support team

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

cds-question@unistra.frlate-type-starschemical-abundancesline-intensitiesIt is known that the surface lithium abundances of field solar-analog G dwarfs show a large dispersion of >~2dex (among which our Sun is located at the lower end) despite the similarity of stellar parameters, and planet-host stars tend to show comparatively lower Li abundances in the narrow Teff range. To investigate the reason for these phenomena, an extensive study of Li abundances and their dependence on stellar parameters was carried out for a homogeneous sample of 118 selected solar analogs based on high-dispersion spectra obtained at Okayama Astrophysical Observatory.2007A&A...468..663Thttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/468/663CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toI/239 : The Hipparcos and Tycho Catalogues (ESA 1997)J/AJ/105/2299 : Li abundance of solar-type stars. II. (Soderblom+, 1993)J/A+A/371/943 : Lithium abundances for 185 main-sequence stars (Chen+, 2001)J/A+A/409/251 : Li abundances and velocities in F and G stars (Mallik+, 2003)J/MNRAS/349/757 : Masses, ages and metallicities of F-G dwarfs (Lambert+, 2004)J/PASJ/57/45 : Lithium abundances of F-K stars (Takeda+, 2005)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/468/663https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/468/663http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/468/663https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/468/663https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/468/663http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/468/663GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/468/663/stars (All parameters of the stars studied)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/468/663/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/468/663/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/468/663/stars?GETtext/xml+votable180.050000true4.6734167-8.05263890.0055555555555555566/222 313 414 417 634 742 1058 2032 2072 2366 2456 2476 2697 3307 3398 3691 3919 4128 4241 4313 4437 4665 5073 5263 5522 5699 5726 5858 6087 6269 6325 6409 6522-6523 6612 6705 7052 7217 7326 7978 8103 8286 8993 9492 9883 10400 10424 10473 10878 11212 11709 12343 12922 13766 13778 14349 14411 14650 15014 15030 15174 15221 15727 16930 17083 17219 17266 17419 17486 17888 18366 18373 18623 19424 19796 19923 21114 21211 21484 21516 21594 21940 22313 22355 22746 22779 23123 23150 23177 23429 23511 23545-23546 23583 24178 25966 26496 27254 27750 27757 28282 28362 28961 29513 30123 30127 30878 31029 31287 32575 32585 32617 36057 36590 40317 40892 40932https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/468/663?format=asciiOpticaldefaultJ/A+A/468/663/starsAll parameters of the stars studiedrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHIPHIP (Cat. <I/239>) numbermeta.id;meta.mainintTeff(standard) effective temperatureKphys.temperature.effectivefloatlogg(standard) logarithmic surface gravitylog(cm.s**-2)phys.gravityfloatvt(standard) microturbulent velocitykm/sphys.velocfloat[Fe/H]s(standard) Fe abundance (A-7.50)log(Sun)phys.abund.FefloatDTeffDifferential Teff relative to the Sun (Teff_{sun}_=5761.0)Kphys.temperature;arith.difffloatDloggDifferential logg relative to the Sun (logg_{sun}_=4.435)log(cm.s**-2)phys.gravityfloatDvtDifferential microturbulent velocity relative to the Sun (vt_{sun}_=1.00)km/sphys.veloc;arith.difffloatD[Fe/H]Differential [Fe/H] relative to the Sun ([Fe/H]_{sun}_=-0.007)phys.abund.FefloatVMAGAbsolute visual magnitude (from table 1)magphys.magAbs;em.opt.VfloatBCBolometric correction (Alonso et al.'s, 1995A&A...297..197A, table 4)magphot.mag.bcfloatMbolBolometric magnitude (=VMAG+BC)magphys.magAbs.bolfloatlogLLogarithmic luminositylog(solLum)phys.luminosityfloatMassStellar mass derived from evolution tracksolMassphys.massfloatE_MassPossible error in Mass on the upper sidesolMassstat.error;stat.maxfloate_MassPossible error in Mass on the lower sidesolMassstat.error;phys.massfloatM(iso)Stellar mass derived from isochronessolMassphys.massfloatlogg(TLM)Theorerical logg derived from Teff, L, and Masslog(cm.s**-2)phys.gravityfloatlogAgeStellar age derived from evolutionary track (adopted)log(yr)time.agefloatE_logAgePossible error in logAge on the upper sidelog(yr)stat.error;stat.maxfloate_logAgePossible error in logAge on the lower sidelog(yr)stat.error;time.agefloatq_logAge[ABC] Reliability of age(trk) (A: high, B: moderate, C: poor)meta.code.qual;time.agecharlogAge(iso)Stellar age derived from isochrones (for reference)log(yr)time.agefloatVrmMacrobroadening velocity (rotation + macroturbulence)km/sphys.velocfloatA(Si)Si abundance derived from 6080-6089 fitphys.abundfloatA(Ti)Ti abundance derived from 6080-6089 fitphys.abundfloatA(V)V abundance derived from 6080-6089 fitphys.abundfloatA(Fe)Fe abundance derived from 6080-6089 fitphys.abund.FefloatA(Co)Co abundance derived from 6080-6089 fitphys.abundfloatA(Ni)Ni abundance derived from 6080-6089 fitphys.abundfloat[Si/H]A(Si)[star]-A(Si)[Sun/Moon=7.455]log(Sun)phys.abundfloat[Ti/H]A(Ti)[star]-A(Ti)[Sun/Moon=4.986]log(Sun)phys.abundfloat[V/H]A(V)[star] -A(V)[Sun/Moon=3.908]log(Sun)phys.abundfloat[Fe/H]A(Fe)[star]-A(Fe)[Sun/Moon=7.534]log(Sun)phys.abund.Fefloat[Co/H]A(Co)[star]-A(Co)[Sun/Moon=4.798]log(Sun)phys.abundfloat[Ni/H]A(Ni)[star]-A(Ni)(Sun/Moon=6.367]log(Sun)phys.abundfloatq_EW(Li)[abx] Quality flag (a: well, b: poor, x: indeterminable)meta.code.qualcharEW(Li)EW(Li 6708) computed from A(LTE) (fitting solution)mAspect.line.eqWidth;meta.modelledfloatl_A(Li)[<] for the upper-limit casemeta.code.errorcharA(Li)Non-LTE Li abundance (=A(LTE)+d(NLTE))phys.abundfloatd(NLTE)? non-LTE correction (not given for the upper-limit case)arith.factorfloatnullableEWsDisplay the equivalent widths of all lines measured for this starmeta.ref.urlcharRAJ2000Right ascension ICRS (J1991.25) (1)pos.eq.ra;meta.mainDEJ2000Declination ICRS (J1991.25) (1)pos.eq.dec;meta.mainplxTrigonometric parallax (1)maspos.parallax.trigfloatpmRAProper motion in alpha direction (1)mas/yrpos.pm;pos.eq.radoublepmDEProper motion in delta direction (1)mas/yrpos.pm;pos.eq.decdoubleHRVHeliocentric radial velocity (from table 1)km/sspect.dopplerVeloc;pos.heliocentricfloatRmMean galactocentric distancekpcpos.distance;stat.meanfloatzmMaximum separation from the galactic planekpcpos.cartesian.z;pos.galacticfloateOrbital eccentricitysrc.orbital.eccentricityfloatUlsrSpace velocity in radial direction relative to LSRkm/sphys.veloc;pos.cartesian.xfloatVlsrSpace velocity in tangential direction relative to LSRkm/sphys.veloc;pos.cartesian.yfloatWlsrSpace velocity in vertical direction relative to LSRkm/sphys.veloc;pos.cartesian.zfloatvlsrSpeed relative to LSR [= sqrt(U^2^+V^2^+W^2^)]km/sphys.veloc;pos.lsrfloatSimbadSimbad column added by the CDScharJ/A+A/468/663/table3EWs of Fe I/Fe II lines and resulting Fe abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintStarStar name (Sun/Moon or HIP NNNNNN)meta.id;meta.maincharLineLine No. (cf. Takeda et al. 2005, Cat. <J/PASJ/57/27>)meta.id;spect.lineintElem26.00 for Fe I, 26.01 for Fe IImeta.notefloatlambdaLine wavelength0.1nmem.wl;spect.linedoubleEP(low)Excitation potential of the lower leveleVphys.atmol.excitation;phys.atmol.levelfloatloggflog(gf) valuestat.value;arith.zpfloatEW? Fe line equivalent width0.1pmspect.line.eqWidthfloatnullableA(Fe)? Line-by-line Fe abundancephys.abund.Fefloatnullable