J/A+A/275/101ivo://CDS.VizieR/J/A+A/275/101doi:10.26093/cds/vizier.32750101CDSEdvardsson B.Andersen J.Gustafsson B.Lambert D.L.Nissen P.E.,Tomkin J.2018-01-08T06:38:14Z1999-02-26T14:46:53ZCDS support team

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

cds-question@unistra.frchemical-abundancesline-intensitiesstellar-agesFrom high resolution, high S/N spectroscopic observations of carefully selected northern and southern stars, abundances of O, Na, Mg, Al, Si, Ca, Ti, Fe, Ni, Y, Zr, Ba and Nd, as well as photometric ages, are derived for 189 nearby field F and G stars.1993A&A...275..101Ehttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/275/101CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+AS/102/603 : Chemical evolution of galactic disk II. (Edvardsson+ 1993)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/275/101https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/275/101http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/275/101https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/275/101https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/275/101http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/275/101GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/275/101/stars (Fundamental data and chemical abundances of 14 species for the programme stars)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/275/101/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/275/101/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/275/101/stars?GETtext/xml+votable180.050000true2.170575836.6271250.0055555555555555566/706 934 1247 1341 1531 1808 2472 2476 2650 3020 3036 3085 3118 4468 4808 4854 5053 5154 5266 5304 5339 5522 5531 5718 5836 5932 6056 6130 6153 6539 6926 7238 7390 8210 8476 8716 8814 8845 9125 9403 9476 9483 9835 10375 10598 10812 10899 11150 11620 11644 11691 11773 12271 12337 12704 13474 13478 13620 14146 14180 14459 14534 14901 15118 15356 15562 15620 16412 16453 16883 17047 17171 17576 17588 17606 17695 17744 17860 18002 18615 19217 19312 19323 19547 19585 19745 20145 20402 20446 20739 21060 21696 21809 21864 21989 22120 22180 22300 22355 22594 22654 22823 22841 23096 23161 23190 23201 23938 23974 24029 24151 24160 24536 24924 24951 25192 25198 25444 25491 25862 25869 26521 26657 26676 26963 26975 27975 28494 28763 29136 29347 30576 30798 30825 30848 31048 31172 31346 31478 31503 31768 32192 32357 32619 33211 33224 33273 33552 34994 35064 35080 35442 36145 36564 36762 37585 37831 38918 38966 39490 39709 39926 40716 40722 40932 41763-41764 41941 42253 42326 42486 43001 43074 43544 43595 44180 44879 45485 45865 46022 46053 46829 47377 47407 47740 48226 48367 49106 49114https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/275/101?format=asciidefaultJ/A+A/275/101/starsFundamental data and chemical abundances of 14 species for the programme starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar catalogue, HR or HDmeta.id;meta.maincharprimaryTeffEffective temperatureKphys.temperature.effectiveintlog.gLogarithmic surface gravitylog(cm.s**-2)phys.gravityfloat[Me/H]overall photometric metallicity derived for the stars, normalized on the Sun (1)log(Sun)phys.abundfloatu_[Me/H]Uncertainty flag (:) on Me/H (2)meta.code.error;phys.abundchar[Fe/H]resulting spectroscopic iron abundance (derived from lines of Fe I), normalized to the Sunlog(Sun)phys.abund.FefloatRHeliocentric distancepcpos.distance;pos.heliocentricfloatUHeliocentric velocity (U is positive towards the galactic anti-centre),km/sphys.veloc;pos.cartesian.xfloatVHeliocentric velocity (V is positive in the direction of circular motion)km/sphys.veloc;pos.cartesian.yfloatWHeliocentric velocity (W is positive towards the galactic north pole)km/sphys.veloc;pos.cartesian.zfloatRpPerigalactic distancekpcpos.distance;src.orbitalfloatRmStraight mean of the perigalactic and the apogalactic distanceskpcpos.distance;src.orbitalfloatZmaxMaximum distance from the galactic planekpcpos.distance;src.orbitalfloateOrbital eccentricity as projected on the galactic planesrc.orbital.eccentricity;pos.galacticfloatlog.age? Logarithm of the stellar age (in Gigayears) determined from isochrones (3)log(Gyr)time.agefloatnullableRemRemarks (4)meta.notechar[FeI/H]Chemical abundance (normalized to the Sun)log(Sun)phys.abundfloat[OI/H]? Chemical abundance (normalized to the Sun)log(Sun)phys.abundfloatnullable[NaI/H]? Chemical abundance (normalized to the Sun)log(Sun)phys.abundfloatnullable[MgI/H]? Chemical abundance (normalized to the Sun)log(Sun)phys.abundfloatnullable[AlI/H]? Chemical abundance (normalized to the Sun)log(Sun)phys.abundfloatnullable[SiI/H]? Chemical abundance (normalized to the Sun)log(Sun)phys.abundfloatnullable[CaI/H]? Chemical abundance (normalized to the Sun)log(Sun)phys.abundfloatnullable[TiI/H]? Chemical abundance (normalized to the Sun)log(Sun)phys.abundfloatnullable[FeII/H]? Chemical abundance (normalized to the Sun)log(Sun)phys.abundfloatnullable[NiI/H]? Chemical abundance (normalized to the Sun)log(Sun)phys.abundfloatnullable[YII/H]? Chemical abundance (normalized to the Sun)log(Sun)phys.abundfloatnullable[ZrII/H]? Chemical abundance (normalized to the Sun)log(Sun)phys.abundfloatnullable[BaII/H]? Chemical abundance (normalized to the Sun)log(Sun)phys.abundfloatnullable[NdII/H]? Chemical abundance (normalized to the Sun)log(Sun)phys.abundfloatnullable[alpha/H]= 0.25([Mg/H] + [Si/H] + [Ca/H] + [Ti/H])log(Sun)phys.abundfloatSimbadSimbad column added by the CDSchar_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/275/101/table8Atomic line data and solar equivalent widthsELine excitation energyeVphys.atmol.excitation;spect.linefloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElementLine identification: chemical element and ionization stagephys.atmol.elementcharLambdaWavelength (Angstroms)0.1nmem.wlfloatlog.gfLog gf (oscillator strength)phys.absorption.coeff;arith.zpfloatFactorEnhancement factor to the "classical van der Waals damping Gamma_6"arith.factor;phys.dampingfloatDampingRadiation damping constantHzphys.absorptiondoubleWSolar flux spectrum equivalent width (milliAngstrom). (1)0.1pmspect.line.eqWidthfloatSourcefor Solar equivalent width: E=ESO spectrum, M=McDonald spectrummeta.id;instr.telchar