J/PASJ/59/335ivo://CDS.VizieR/J/PASJ/59/335doi:10.26093/cds/vizier/bj-1v-afCDSTakeda Y.2026-03-17T20:04:52Z2008-09-12T12:30:49ZCDS support team

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

cds-question@unistra.frlate-type-starsdwarf-starschemical-abundancesline-intensitiesstellar-massesstellar-agesThe properties of 160 F, G, and K disk dwarfs/subgiants (including 27 planet-host stars) mostly within -0.6<~[Fe/H]<~+0.4, the Okayama Astrophysical Observatory spectrum collection of which had been made open to the public recently, were extensively investigated with particular attention to determining (1) the mass and the age with the help of theoretical stellar evolution calculations, (2) the kinematic parameters of orbital motions in the Galaxy, and (3) the abundances of 15 elements (Na, Mg, Al, Si, S, Ca, Sc, Ti, V, Cr, Mn, Co, Ni, Cu, and Zn) by analyzing the spectra in this database. The resulting characteristics are discussed in terms of several relevant topics of interest, such as a validity check for assuming LTE, the [X/Fe] vs. [Fe/H] diagram containing information on the chemical evolution of the Galactic disk, the age-metallicity-kinematics relation, and the difference/similarity between stars with and without planets.2007PASJ...59..335Thttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/PASJ/59/335CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/PASJ/57/13 : High-dispersion spectra of nearby F-K stars (Takeda+, 2005)J/PASJ/57/27 : Atmospheric parameters of nearby F-K stars (Takeda+, 2005)J/PASJ/57/45 : Lithium abundances of F-K stars (Takeda+, 2005)J/PASJ/57/65 : CNO abundances of solar-type stars (Takeda+, 2005)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PASJ/59/335https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PASJ/59/335http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PASJ/59/335https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/PASJ/59/335https://vizier.iucaa.in/viz-bin/votable?-source=J/PASJ/59/335http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/PASJ/59/335GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/PASJ/59/335/catalog (Results on program stars: astrophysical parameters, abundances, kinematic parameters)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/PASJ/59/335/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/PASJ/59/335/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/PASJ/59/335/catalog?GETtext/xml+votable180.050000true1.5647558.43669440.0055555555555555566/679 684 706 819 934 1341 2472 2476 2650 2923 3006 3020 3036 3118 3639 4468 4808 4839 4854 5009 5154 5266 5304 5339 5522 5531 5670 5718 5836 6056 6130 6308 6926 7238 7390 8476 8602 8716 8788 8790 8843 8845 9072 9125 9403 9476 9835 9843 10375 10598 10812 10899 11290 11620 11691 11773 12146 12337 12464 12890 12899 12944 13474 13620 14146 14180 14459 14539 14573 15030 15118 15174 15356 15620 15962 16069 16883 17171 17425 17576 17588 17606 17730 17860 18002 18139 18614 18821 19312 19323 19585 20145 20278 20440 20446 21696 21864 22036 22120 22180 22300 22594 22654 22878 23013 23190 23201 23230 23974 24019 24151 24160 24212 24920 24924 24951 25198 25407 25862 25869 26462 26521 26575 26676 26963 26975 27088 28122 28494 28605 28664 28763 29541 30576 30665 30798 30848 30965 30989 31478 31751 32067 32192 32619 32645 36564 36664 36697 36723 36762 40442 40692 40716 40823 40932 44243 44879 48105 49114https://cdsarc.cds.unistra.fr/viz-bin/moc/J/PASJ/59/335?format=asciidefaultJ/PASJ/59/335/catalogResults on program stars: astrophysical parameters, abundances, kinematic parametersNameStar namemeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintn_HD[P] 'P' when star harbors planet(s)meta.notecharHDHD number of the starmeta.id;meta.mainintprimaryHR? HR number of the starmeta.idintnullableHIP? HIP number of the starmeta.idintnullableSpTypeMK spectral typesrc.spTypecharTeffEffective temperature (1)Kphys.temperature.effectiveintloggSurface gravity (1)log(cm.s**-2)phys.gravityfloatvtMicroturbulent velocity (1)km/sphys.velocfloat[Fe/H]Metallicity (1)log(Sun)phys.abund.ZfloatlogLStellar luminosity derived as -0.4(M_bol_-4.75)log(solLum)phys.luminosityfloatMassMass (2)solMassphys.massfloatlogAgeAge (2)log(yr)time.agefloatq_logAge[ABC] Quality flag showing the reliability of age (see Sect. 2.1 for more details) (3)meta.code.qual;time.agecharV(LSR)Space speed relative to the LSR (G1)km/sphys.velocfloatAbunDisplay the detailed abundance corrections with hyper-fine splittingmeta.ref.urlcharSimbadSimbad column added by the CDScharTeff2Effective temperature (1)Kphys.temperature.effectivefloatlogg2logarithmic surface gravity (1)log(cm.s**-2)phys.gravityfloatvt2microturbulent velocity (1)km/sphys.velocfloat[Fe/H]2Fe abundance relative to the Sun (1)log(Sun)phys.abund.FefloatVMAG2Absolute visual magnitude (2)magphys.magAbs;em.opt.VfloatBC2Bolometric correction (2)magphot.mag.bcfloatMbol2Bolometric magnitude (2)magphot.mag.bolfloatlogL2logarithmic luminositylog(solLum)phys.luminosityfloatM(trk)Stellar mass derived from evolutionary track (3)solMassphys.massfloatE_M(trk)Possible error in M(trk) on the upper sidesolMassstat.error;stat.maxfloate_M(trk)Possible error in M(trk) on the lower sidesolMassstat.errorfloatM(iso)Stellar mass derived from isochronessolMassphys.massfloatlogg(TLM)Theorerical logg derived from Teff, L, and M(trk)log(cm.s**-2)phys.gravityfloatlogAge(trk)log(stellar age) derived from evolutionary track (3)log(yr)arith.zpfloatE_logAge(trk)Possible error in logAge(trk) on the upper sidelog(yr)stat.error;stat.maxfloate_logAge(trk)Possible error in logAge(trk) on the lower sidelog(yr)stat.errorfloatq_logAge(trk)Reliability of age(trk) (4)meta.code.qualcharlogAge(iso)log(stellar age) derived from isochroneslog(yr)arith.zpfloatPapIIShow the stellar parameters from PaperII (2005, Cat. J/PASJ/57/27)meta.ref.urlcharRAJ2000Right ascension (J2000, Ep=1991.25, HIP)pos.eq.ra;meta.mainDEJ2000Declination (J2000, Ep=1991.25, HIP)pos.eq.dec;meta.mainplxParallax (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 2 of Paper I, Cat. J/PASJ/57/13)km/sspect.dopplerVeloc;pos.heliocentricfloatRmMean galactocentric distancekpcpos.distance;src.orbitalfloatzmMaximum separation from the galactic planekpcsrc.orbitalfloateGalactocentric orbital eccentricitysrc.orbital.eccentricity;pos.galactocentricfloatUlsrSpace 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.zfloatPapIShow tables from PaperI (2005, Cat. J/PASJ/57/13) for this starmeta.ref.urlchar[Na/H]Na abundance relative to the Sunlog(Sun)phys.abundfloat[Mg/H]Mg abundance relative to the Sun (MgI 8806 fit)log(Sun)phys.abundfloat[Al/H]? Al abundance relative to the Sunlog(Sun)phys.abundfloatnullable[Si/H]Si abundance relative to the Sunlog(Sun)phys.abundfloat[S/H]? S abundance relative to the Sun (SI 8684 fit)log(Sun)phys.abundfloatnullable[Ca/H]Ca abundance relative to the Sunlog(Sun)phys.abundfloat[ScI/H]? Sc abundance relative to the Sun (from ScI)log(Sun)phys.abundfloatnullable[ScII/H]Sc abundance relative to the Sun (from ScII)log(Sun)phys.abundfloat[TiI/H]Ti abundance relative to the Sun (from TiI)log(Sun)phys.abundfloat[TiII/H]Ti abundance relative to the Sun (from TiII)log(Sun)phys.abundfloat[VI/H]? V abundance relative to the Sun (from VI)log(Sun)phys.abundfloatnullable[VII/H]? V abundance relative to the Sun (from VII)log(Sun)phys.abundfloatnullable[CrI/H]Cr abundance relative to the Sun (from CrI)log(Sun)phys.abundfloat[CrII/H]Cr abundance relative to the Sun (from CrII)log(Sun)phys.abundfloat[Mn/H]? Mn abundance relative to the Sunlog(Sun)phys.abundfloatnullable[Co/H]Co abundance relative to the Sunlog(Sun)phys.abundfloat[Ni/H]Ni abundance relative to the Sunlog(Sun)phys.abundfloat[Cu/H]? Cu abundance relative to the Sunlog(Sun)phys.abundfloatnullable[Zn/H]? Zn abundance relative to the Sunlog(Sun)phys.abundfloatnullableA(Mg)Mg abundance from 8806 fit (normalisation of H=12.00)phys.abundfloatEW(Mg)EW(MgI 8806.8) inversely computed from A(Mg)0.1pmspect.line.eqWidth;meta.modelledfloatA(S)S abundance from 8693-5 fit (normalisation of H=12.00)phys.abundfloatEW(S1)? EW(SI 8693.1) inversely computed from A(S)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEW(S2)? EW(SI 8693.9) inversely computed from A(S)0.1pmspect.line.eqWidth;meta.modelledfloatnullableEW(S3)? EW(SI 8694.6) inversely computed from A(S)0.1pmspect.line.eqWidth;meta.modelledfloatnullableJ/PASJ/59/335/mabundAverage abundances (from tablee3)NlineNumber of lines for the speciesmeta.numberintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordinto_<delA>Number of lines actually adopted for computing the averaged abundancesmeta.numberint<delA>Average differential abundance (star-Sun)phys.abundfloate_<delA>rms uncertainty on <delA>stat.errorfloatFileNameName of the file with individual measurements in subdirectory cmbmeta.id;meta.filecharHDHD numbermeta.id;meta.mainintIonIon code (G2)meta.code;phys.atmol.ionStagefloatJ/PASJ/59/335/xhcorCorrections on the final (line-averaged) results of [ScII/H], [VI/H], [MnI/H] and [CoI/H] caused by inclusion of the hyper-fine splitting effect for each of the relevant lines (from tablee4)HDHD numbermeta.id;meta.mainintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTeffEffective temperatureKphys.temperature.effectivefloatlogglogarithmic surface gravitylog(cm.s**-2)phys.gravityfloatvtMicroturbulent velocitykm/sphys.velocfloat[Fe/H]Fe abundance relative to the Sunlog(Sun)phys.abundfloatIonIon code (G2) (1)phys.abundfloat[X/H](hfs)final [X/H] value obtained with hfsphys.abundfloat[X/H](nohf)final [X/H] value obtained without hfsphys.abundfloatdeltahfs correction ([X/H](hfs)-[X/H](nohf))phys.abundfloatJ/PASJ/59/335/lgf*Wavelength and the loggf data of each hyper-fine splitting (hfs) component (from tablee4)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaLine wavelength0.1nmem.wl;spect.lineinto_IonNumber of hyperfine componentsmeta.numberintIonIon code (G2) (1)meta.code;phys.atmol.ionStagefloatlam.hfWavelength of the hyperfine components0.1nmem.wldoublechi? lower excitation potentialeVphys.atmol.excitation;stat.minfloatnullableloggflog of (statistical weight times oscillator strength)arith.zpfloatJ/PASJ/59/335/difResults of abundance corrections caused by inclusion of the hyper-fine splitting (hfs) effect for the relevant line (from tablee4)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIonIon code (G2) (1)meta.code;phys.atmol.ionStagefloatlambdaLine wavelength0.1nmem.wl;spect.lineintHDHD number (0 for Sun)meta.id;meta.mainintTeffEffective temperatureKphys.temperature.effectivefloatloggLogarithmic surface gravitylog(m.s**-2)phys.gravityfloatvtMicroturbulent velocitykm/sphys.velocfloat[Fe/H]Fe abundance relative to the Sunphys.abund.FefloatEWEquivalent width of the line0.1pmspect.line.eqWidthfloatA(hfs)Abundance obtained with hyperfine splittingphys.abundfloatA(nohf)Abundance obtained without hyperfine splittingphys.abundfloatdeltahfs correction defined as A(hfs)-A(nohf)phys.abundfloat