J/MNRAS/450/397ivo://CDS.VizieR/J/MNRAS/450/397doi:10.26093/cds/vizier.74500397CDSTakeda Y.Tajitsu A.2024-08-14T20:22:03Z2019-12-16T09:05:13ZCDS support team

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

cds-question@unistra.frgiant-starseffective-temperaturechemical-abundancesstellar-radiistellar-massesspectroscopyline-intensitiesThanks to the recent very high precision photometry of red giants from satellites such as Kepler, precise mass and radius values as well as accurate information of evolutionary stages are already established by asteroseismic approach for a large number of G-K giants. Based on the high-dispersion spectra of selected such 55 red giants in the Kepler field with precisely known seismic parameters (among which parallaxes are available for nine stars), we checked the accuracy of the determination method of stellar parameters previously applied to many red giants by Takeda et al. (2008PASJ...60..781T), since it may be possible to discriminate their complex evolutionary status by using the surface gravity versus mass diagram. We confirmed that our spectroscopic gravity and the seismic gravity satisfactorily agree with each other (to within ~0.1 dex) without any systematic difference. However, the mass values of He-burning red clump giants derived from stellar evolutionary tracks (~2-3 M_{sun}_) were found to be markedly larger by ~50 percent compared to the seismic values (~1-2 M_{sun}_) though such discrepancy is not seen for normal giants in the H-burning phase, which reflects the difficulty of mass determination from intricately overlapping tracks on the luminosity versus effective temperature diagram. This consequence implies that the mass results of many red giants in the clump region determined by Takeda et al. are likely to be significantly overestimated. We also compare our spectroscopically established parameters with recent literature values, and further discuss the prospect of distinguishing the evolutionary status of red giants based on the conventional (i.e. non-seismic) approach.2015MNRAS.450..397Thttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/450/397CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toV/133 : Kepler Input Catalog (Kepler Mission Team, 2009)J/PASJ/57/27 : Atmospheric parameters of nearby F-K stars (Takeda+, 2005)J/A+A/540/A143 : Oscillations of red giants observed by Kepler (Mosser+, 2012)J/A+A/543/A160 : Normalized spectra of 82 Kepler red giants (Thygesen+, 2012)J/ApJS/215/19 : APOKASC catalog of Kepler red giants (Pinsonneault+, 2014)J/ApJS/236/42 : Asteroseismology of ~16000 Kepler red giants (Yu+, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/450/397https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/450/397http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/450/397https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/450/397https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/450/397http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/450/397GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/450/397/table1 (Basic data and the resulting parameters of the programme stars)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/450/397/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/450/397/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/450/397/table1?GETtext/xml+votable180.050000true292.504446137.29275190.0055555555555555565/3730 6/14579 14581 14584-14586 14733-14734 14744 14756-14757 14760 14763 14775-14777 14794 14819 14827 14915 14918 14924 14930-14933 14936-14937 14944 14975 15040 15113 15118 15129 15145 15148 15153 15171 15200https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/450/397?format=asciidefaultJ/MNRAS/450/397/table1Basic data and the resulting parameters of the programme starsSourceData source (3)meta.id;instr.telcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNote[ST] Note on results (1)meta.notecharKIC[1726211/12884274] KIC numbermeta.id;meta.mainintprimarymoreindicates broadening velocities and abundances in Table e2 for this starmeta.ref.urlcharKpmag[6.72/11.91] Kepler magnitudemagphot.mag;em.optfloatTeff[4519/5472] Effective temperatureKphys.temperature.effectiveintlogg[2.34/3.75] Logarithmic surface gravitylog(cm.s**-2)phys.gravityfloatvt[0.74/1.46] Microturbulent velocity dispersionkm/sphys.veloc.dispersionfloat[Fe/H][-0.72/0.37] Metallicity (dex)phys.abund.Zfloatnumax[29/630.3] Central frequency of the oscillation power excess {nu}_max_uHzem.freqfloatDnu[3.64/39.7] Large frequency separation {Delta}{nu}uHzem.freq;src.varfloatDPi1[59.51/333.3] Gravity-mode spacing {Delta}{Pi}1stime.periodfloatRseis[2.32/13.65] Asteroseismic radiussolRadphys.size.radiusfloatMseis[0.78/3.49] Asteroseismic masssolMassphys.massfloatloggseis[2.38/3.74] Seismic surface gravitylog(cm.s**-2)phys.gravityfloatvesini[1.6/4] Projected rotational velocity v_e_sinikm/sphys.veloc.rotatfloatClassEvolutionary class determined by Mosser et al. (2012, J/A+A/540/A143) (2)src.classcharLabelStar label used in Table e1meta.codecharEWsEquivalents widths and abundances in Table e1meta.ref.urlcharSimbadSimbad 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/MNRAS/450/397/tablee1EWs of Fe I/Fe II lines and corresponding Fe abundancerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLine[102/2014] Line number (cf. Takeda et al. 2005, J/PASJ/57/27)meta.numberintElem[26/26.01] Element code (26.00 for Fe I, 26.01 for Fe II)phys.atmol.numberfloatlambda[4365.8/7495.06] Line (air) wavelength ({AA})0.1nmem.wl;spect.linedoubleEP(low)[0.087/6.724] Excitation potential of the lower leveleVphys.atmol.excitation;phys.atmol.levelfloatloggf[-6.477/0.083] log(gf) value (dex)stat.value;arith.zpfloatEW(Fe)1s[0/118.9] Fe line equivalent width for KIC 01726211 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)1s[0/7.18] Line-by-line Fe abundance for KIC 01726211 (dex) (1)phys.abund.FefloatEW(Fe)2[0/119.3] Fe line equivalent width for KIC 02013502 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)2[0/7.78] Line-by-line Fe abundance for KIC 02013502 (dex) (1)phys.abund.FefloatEW(Fe)3[0/119.8] Fe line equivalent width for KIC 02303367 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)3[0/7.91] Line-by-line Fe abundance for KIC 02303367 (dex) (1)phys.abund.FefloatEW(Fe)4[0/119.2] Fe line equivalent width for KIC 02424934 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)4[0/7.57] Line-by-line Fe abundance for KIC 02424934 (dex) (1)phys.abund.FefloatEW(Fe)5[0/119.3] Fe line equivalent width for KIC 02448225 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)5[0/8.05] Line-by-line Fe abundance for KIC 02448225 (dex) (1)phys.abund.FefloatEW(Fe)6s[0/119.1] Fe line equivalent width for KIC 02714397 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)6s[0/7.26] Line-by-line Fe abundance for KIC 02714397 (dex) (1)phys.abund.FefloatEW(Fe)7[0/117.7] Fe line equivalent width for KIC 03217051 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)7[0/8.08] Line-by-line Fe abundance for KIC 03217051 (dex) (1)phys.abund.FefloatEW(Fe)8[0/119] Fe line equivalent width for KIC 03455760 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)8[0/7.77] Line-by-line Fe abundance for KIC 03455760 (dex) (1)phys.abund.FefloatEW(Fe)9[0/118.3] Fe line equivalent width for KIC 03730953 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)9[0/7.71] Line-by-line Fe abundance for KIC 03730953 (dex) (1)phys.abund.FefloatEW(Fe)10s[0/115.1] Fe line equivalent width for KIC 03744043 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)10s[0/7.35] Line-by-line Fe abundance for KIC 03744043 (dex) (1)phys.abund.FefloatEW(Fe)11[0/118.9] Fe line equivalent width for KIC 03758458 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)11[0/7.83] Line-by-line Fe abundance for KIC 03758458 (dex) (1)phys.abund.FefloatEW(Fe)12[0/119.9] Fe line equivalent width for KIC 04036007 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)12[0/7.4] Line-by-line Fe abundance for KIC 04036007 (dex) (1)phys.abund.FefloatEW(Fe)13[0/118.5] Fe line equivalent width for KIC 04044238 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)13[0/8.05] Line-by-line Fe abundance for KIC 04044238 (dex) (1)phys.abund.FefloatEW(Fe)14[0/111.4] Fe line equivalent width for KIC 04243623 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)14[0/7.48] Line-by-line Fe abundance for KIC 04243623 (dex) (1)phys.abund.FefloatEW(Fe)15[0/119.2] Fe line equivalent width for KIC 04243796 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)15[0/7.97] Line-by-line Fe abundance for KIC 04243796 (dex) (1)phys.abund.FefloatEW(Fe)16[0/118.5] Fe line equivalent width for KIC 04351319 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)16[0/8.11] Line-by-line Fe abundance for KIC 04351319 (dex) (1)phys.abund.FefloatEW(Fe)17[0/118.2] Fe line equivalent width for KIC 04445711 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)17[0/7.38] Line-by-line Fe abundance for KIC 04445711 (dex) (1)phys.abund.FefloatEW(Fe)18[0/119.6] Fe line equivalent width for KIC 04770846 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)18[0/7.77] Line-by-line Fe abundance for KIC 04770846 (dex) (1)phys.abund.FefloatEW(Fe)19[0/117.5] Fe line equivalent width for KIC 04902641 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)19[0/7.77] Line-by-line Fe abundance for KIC 04902641 (dex) (1)phys.abund.FefloatEW(Fe)20[0/118.6] Fe line equivalent width for KIC 04952717 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)20[0/8] Line-by-line Fe abundance for KIC 04952717 (dex) (1)phys.abund.FefloatEW(Fe)21[0/118.4] Fe line equivalent width for KIC 05000307 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)21[0/7.46] Line-by-line Fe abundance for KIC 05000307 (dex) (1)phys.abund.FefloatEW(Fe)22[0/119.6] Fe line equivalent width for KIC 05033245 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)22[0/7.81] Line-by-line Fe abundance for KIC 05033245 (dex) (1)phys.abund.FefloatEW(Fe)23[0/115.2] Fe line equivalent width for KIC 05088362 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)23[0/7.92] Line-by-line Fe abundance for KIC 05088362 (dex) (1)phys.abund.FefloatEW(Fe)24[0/114.7] Fe line equivalent width for KIC 05128171 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)24[0/7.84] Line-by-line Fe abundance for KIC 05128171 (dex) (1)phys.abund.FefloatEW(Fe)25[0/119.7] Fe line equivalent width for KIC 05266416 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)25[0/7.68] Line-by-line Fe abundance for KIC 05266416 (dex) (1)phys.abund.FefloatEW(Fe)26[0/119.1] Fe line equivalent width for KIC 05307747 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)26[0/7.77] Line-by-line Fe abundance for KIC 05307747 (dex) (1)phys.abund.FefloatEW(Fe)27[0/117.6] Fe line equivalent width for KIC 05530598 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)27[0/8.25] Line-by-line Fe abundance for KIC 05530598 (dex) (1)phys.abund.FefloatEW(Fe)28[0/117.9] Fe line equivalent width for KIC 05723165 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)28[0/7.65] Line-by-line Fe abundance for KIC 05723165 (dex) (1)phys.abund.FefloatEW(Fe)29[0/118.4] Fe line equivalent width for KIC 05737655 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)29[0/7.12] Line-by-line Fe abundance for KIC 05737655 (dex) (1)phys.abund.FefloatEW(Fe)30[0/119.9] Fe line equivalent width for KIC 05806522 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)30[0/7.91] Line-by-line Fe abundance for KIC 05806522 (dex) (1)phys.abund.FefloatEW(Fe)31[0/118.9] Fe line equivalent width for KIC 05866737 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)31[0/7.58] Line-by-line Fe abundance for KIC 05866737 (dex) (1)phys.abund.FefloatEW(Fe)32[0/119.6] Fe line equivalent width for KIC 05990753 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)32[0/7.95] Line-by-line Fe abundance for KIC 05990753 (dex) (1)phys.abund.FefloatEW(Fe)33[0/116.2] Fe line equivalent width for KIC 06117517 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)33[0/8.17] Line-by-line Fe abundance for KIC 06117517 (dex) (1)phys.abund.FefloatEW(Fe)34[0/119] Fe line equivalent width for KIC 06144777 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)34[0/7.97] Line-by-line Fe abundance for KIC 06144777 (dex) (1)phys.abund.FefloatEW(Fe)35[0/116.5] Fe line equivalent width for KIC 06276948 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)35[0/7.92] Line-by-line Fe abundance for KIC 06276948 (dex) (1)phys.abund.FefloatEW(Fe)36[0/118] Fe line equivalent width for KIC 07205067 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)36[0/7.76] Line-by-line Fe abundance for KIC 07205067 (dex) (1)phys.abund.FefloatEW(Fe)37[0/118.2] Fe line equivalent width for KIC 07581399 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)37[0/7.74] Line-by-line Fe abundance for KIC 07581399 (dex) (1)phys.abund.FefloatEW(Fe)38[0/119.7] Fe line equivalent width for KIC 08378462 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)38[0/7.83] Line-by-line Fe abundance for KIC 08378462 (dex) (1)phys.abund.FefloatEW(Fe)39[0/102.9] Fe line equivalent width for KIC 08702606 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)39[0/7.59] Line-by-line Fe abundance for KIC 08702606 (dex) (1)phys.abund.FefloatEW(Fe)40[0/117.8] Fe line equivalent width for KIC 08718745 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)40[0/7.5] Line-by-line Fe abundance for KIC 08718745 (dex) (1)phys.abund.FefloatEW(Fe)41[0/118.3] Fe line equivalent width for KIC 09173371 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)41[0/7.71] Line-by-line Fe abundance for KIC 09173371 (dex) (1)phys.abund.FefloatEW(Fe)42[0/118.3] Fe line equivalent width for KIC 11819760 (m{AA}) (1)0.1pmspect.line.eqWidthfloatlogeps(Fe)42[0/7.6] Line-by-line Fe abundance for KIC 11819760 (dex) (1)phys.abund.FefloatEW(Fe)1n[0/117.5] Fe line equivalent width for KIC 01726211 (m{AA}) (2)0.1pmspect.line.eqWidthfloatlogeps(Fe)1n[0/7.25] Line-by-line Fe abundance for KIC 01726211 (dex) (2)phys.abund.FefloatEW(Fe)6n[0/119.1] Fe line equivalent width for KIC 02714397 (m{AA}) (2)0.1pmspect.line.eqWidthfloatlogeps(Fe)6n[0/7.45] Line-by-line Fe abundance for KIC 02714397 (dex) (2)phys.abund.FefloatEW(Fe)10n[0/115.5] Fe line equivalent width for KIC 03744043 (m{AA}) (2)0.1pmspect.line.eqWidthfloatlogeps(Fe)10n[0/7.51] Line-by-line Fe abundance for KIC 03744043 (dex) (2)phys.abund.FefloatEW(Fe)43[0/118.6] Fe line equivalent width for KIC 03748691 (m{AA}) (2)0.1pmspect.line.eqWidthfloatlogeps(Fe)43[0/7.94] Line-by-line Fe abundance for KIC 03748691 (dex) (2)phys.abund.FefloatEW(Fe)44[0/116.8] Fe line equivalent width for KIC 05795626 (m{AA}) (2)0.1pmspect.line.eqWidthfloatlogeps(Fe)44[0/7.1] Line-by-line Fe abundance for KIC 05795626 (dex) (2)phys.abund.FefloatEW(Fe)45[0/117.9] Fe line equivalent width for KIC 06690139 (m{AA}) (2)0.1pmspect.line.eqWidthfloatlogeps(Fe)45[0/7.7] Line-by-line Fe abundance for KIC 06690139 (dex) (2)phys.abund.FefloatEW(Fe)46[0/119] Fe line equivalent width for KIC 08813946 (m{AA}) (3)0.1pmspect.line.eqWidthfloatlogeps(Fe)46[0/7.91] Line-by-line Fe abundance for KIC 08813946 (dex) (3)phys.abund.FefloatEW(Fe)47[0/118.1] Fe line equivalent width for KIC 09705687 (m{AA}) (2)0.1pmspect.line.eqWidthfloatlogeps(Fe)47[0/7.52] Line-by-line Fe abundance for KIC 09705687 (dex) (2)phys.abund.FefloatEW(Fe)48[0/118.6] Fe line equivalent width for KIC 10323222 (m{AA}) (3)0.1pmspect.line.eqWidthfloatlogeps(Fe)48[0/7.92] Line-by-line Fe abundance for KIC 10323222 (dex) (3)phys.abund.FefloatEW(Fe)49[0/119.8] Fe line equivalent width for KIC 10404994 (m{AA}) (3)0.1pmspect.line.eqWidthfloatlogeps(Fe)49[0/7.74] Line-by-line Fe abundance for KIC 10404994 (dex) (3)phys.abund.FefloatEW(Fe)50[0/118.1] Fe line equivalent width for KIC 10426854 (m{AA}) (2)0.1pmspect.line.eqWidthfloatlogeps(Fe)50[0/7.48] Line-by-line Fe abundance for KIC 10426854 (dex) (2)phys.abund.FefloatEW(Fe)51[0/119.1] Fe line equivalent width for KIC 10716853 (m{AA}) (3)0.1pmspect.line.eqWidthfloatlogeps(Fe)51[0/7.65] Line-by-line Fe abundance for KIC 10716853 (dex) (3)phys.abund.FefloatEW(Fe)52[0/116.7] Fe line equivalent width for KIC 11444313 (m{AA}) (2)0.1pmspect.line.eqWidthfloatlogeps(Fe)52[0/7.8] Line-by-line Fe abundance for KIC 11444313 (dex) (2)phys.abund.FefloatEW(Fe)53[0/119.9] Fe line equivalent width for KIC 11569659 (m{AA}) (2)0.1pmspect.line.eqWidthfloatlogeps(Fe)53[0/7.58] Line-by-line Fe abundance for KIC 11569659 (dex) (2)phys.abund.FefloatEW(Fe)54[0/119.5] Fe line equivalent width for KIC 11657684 (m{AA}) (2)0.1pmspect.line.eqWidthfloatlogeps(Fe)54[0/7.82] Line-by-line Fe abundance for KIC 11657684 (dex) (2)phys.abund.FefloatEW(Fe)55[0/119.2] Fe line equivalent width for KIC 12884274 (m{AA}) (3)0.1pmspect.line.eqWidthfloatlogeps(Fe)55[0/7.97] Line-by-line Fe abundance for KIC 12884274 (dex) (3)phys.abund.FefloatJ/MNRAS/450/397/tablee2Broadening velocities and abundances from 6080-6089{AA} fit[Ti/H][-0.63/0.34] Ti abundance log{eps}Ti(star)-log{eps}Ti(Sun:4.986) (dex)phys.abundfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintKIC[1726211/12884274] KIC numbermeta.id;meta.mainintSource[snc] Code indicating the source of spectrum (1)meta.ref;pos.framecharTeff[4519/5472] Effective temperatureKphys.temperature.effectiveintlogg[2.34/3.75] Logarithmic surface gravitylog(cm.s**-2)phys.gravityfloatvt[0.74/1.46] Microturbulent velocitykm/sphys.velocfloat[Fe/H]1[-0.72/0.37] Logarithmic Fe abundance relative to the Sunlog(Sun)phys.abund.FefloatvM[3.11/4.81] Total macrobroadening (Gaussian e-folding width)km/sspect.line.broadfloatvip[2.25/2.69] Instrumental broadening (Gaussian e-folding width)km/sspect.line.broadfloatvrm[2.15/4.25] ip-subtracted macrobroadening [=sqrt(v_M_**2-v_ip_**2)]km/sspect.line.broadfloatvmt[1.79/2.73] Macroturbulence broadening (=4.3-0.67*log g)km/sspect.line.broadfloatvrt[0.91/3.32] Rotational broadening [=sqrt(v_rm_**2-v_mt_**2)]km/sspect.line.broadfloatvesini[1.59/4.02] Finally adopted v sini (=1.01*v_rt_+0.67)km/sphys.veloc.rotatfloatlogeps(Si)[7.05/7.81] Si abundance derived from 6080-6089{AA} fit (dex)phys.abundfloatlogeps(Ti)[4.36/5.32] Ti abundance derived from 6080-6089{AA} fit (dex)phys.abundfloatlogeps(V)[3.23/4.54] V abundance derived from 6080-6089{AA} fit (dex)phys.abundfloatlogeps(Fe)[6.75/7.87] Fe abundance derived from 6080-6089{AA} fit (dex)phys.abund.Fefloatlogeps(Co)[4.22/5.38] Co abundance derived from 6080-6089{AA} fit (dex)phys.abundfloatlogeps(Ni)[5.48/6.85] Ni abundance derived from 6080-6089{AA} fit (dex)phys.abundfloat[Si/H][-0.41/0.35] Si abundance log{eps}Si(star)-log{eps}Si(Sun:7.455) (dex)phys.abundfloat[V/H][-0.68/0.63] V abundance log{eps}V(star)-log{eps}V(Sun:3.908) (dex)phys.abundfloat[Fe/H]2[-0.78/0.34] Fe abundance log{eps}Fe(star)-log{eps}Fe(Sun:7.534) (dex)phys.abund.Fefloat[Co/H][-0.58/0.58] Co abundance log{eps}Co(star)-log{eps}Co(Sun:4.798) (dex)phys.abundfloat[Ni/H][-0.89/0.48] Ni abundance log{eps}Ni(star)-log{eps}Ni(Sun:6.367) (dex)phys.abundfloat