J/A+A/326/751ivo://CDS.VizieR/J/A+A/326/751doi:10.26093/cds/vizier.33260751CDSNissen P.E.Schuster W.J.2017-11-10T11:16:12Z2005-05-26T08:35:04ZCDS support team

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

cds-question@unistra.frchemical-abundancespopulation-ii-starsvisible-astronomymedium-band-photometryTable A1 lists the Stromgren photometry together with color excesses, E(b-y), photometric metallicities, [Fe/H] , calculated from the calibrations of Schuster & Nissen (1989A&A...221...65S), and absolute magnitudes, M(V), and distances derived with the equations of Nissen & Schuster (1991A&A...251..457N) using the photometric metallicities. Table A2 contains coordinates, proper motions and radial velocities for the program stars as well as distances calculated from the calibrations Nissen & Schuster (1991A&A...251..457N) using the spectroscopic metallicities scaled to our photometric [Fe/H] system. Table A3 gives a list of the 209 spectral lines, which were analyzed, arranged element by element. The table contains the wavelength, the excitation potential of the lower level corresponding to the line, the gf-value, the enhancement factor of the classical van der Waals damping constant, the statistical weight of the upper level, and the equivalent widths measured for the two "standard" stars, HD 22879 and HD 76932. Table A4 contains the measured equivalent widths for all program stars. Table A5 gives abundance ratios and kinematical as well as orbital parameters for the program stars. First are given the data for the 16 disk stars, then follows the 14 halo stars.1997A&A...326..751Nhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/326/751CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/326/751https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/326/751http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/326/751https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/326/751https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/326/751http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/326/751GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/326/751/stars (Stars observed (tables A1 and A2 of paper))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/326/751/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/326/751/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/326/751/stars?GETtext/xml+votable180.050000true9.632942-8.3016340.0055555555555555566/200 436 17245 22518 23015 23096 23734 24775 24824 24827 25444 27323 27857 33273 33508 33580 34350 36114 38440 38986 39157 39647 40716 41721 43310 43641 43678 43962 446533.322582951404819e-19 3.852589004194616e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/326/751?format=asciiOpticaldefaultJ/A+A/326/751/starsStars observed (tables A1 and A2 of paper)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameDesignation of starmeta.id;meta.maincharprimaryEWColumn containing the equivalent width in table A4spect.line.eqWidth;meta.tableintnullableVmagVisual magnitude (1)magphot.mag;em.opt.Vfloatb-yColour index (1)magphot.color;em.opt.B;em.opt.Vfloatm1Metallicity index (1)magphot.colorfloatc1Balmer discontinuity index (1)magphot.colorfloatHbeta? H-beta line indexmagspect.index;em.line.HbetafloatnullableE(b-y)? Color excessmagphot.color.excessfloatnullable[Fe/H]Photometric metallicitylog(Sun)phys.abund.ZfloatM(V)? Absolute magnitudemagphys.magAbsfloatnullableDist1Distance (using photometric metallicities)pcpos.distance;pos.heliocentricintSimbadSimbad column added by the CDSmeta.refcharRA1950Right ascension (1950.0)pos.eq.ra;meta.mainDE1950Declination (1950.0)pos.eq.dec;meta.mainEpochEpoch of coordinatesyrtime.epochintpmRAProper motion = 15*mu(alpha)*cos(dec)arcsec/yrpos.pm;pos.eq.rafloatpmDEProper motion = mu(dec)arcsec/yrpos.pm;pos.eq.decfloatHRVHeliocentric radial velocitykm/sspect.dopplerVeloc;pos.heliocentricfloatDist2Distance (using spectroscopic metallicities)pcpos.distance;pos.heliocentricint_RA.icrsRight ascension (ICRS) at Epoch=J2000, proper motions taken into account (computed by VizieR, not part of the original data)pos.eq.ranullableindexed_DE.icrsDeclination (ICRS) at Epoch=J2000, proper motions taken into account (computed by VizieR, not part of the original data)pos.eq.decnullableindexedJ/A+A/326/751/tablea3Atomic line data and equivalent widths for the standard stars HD 22879 and HD 76932recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElementChemical element and ionization stagephys.atmol.ionStage;phys.atmol.ionizationcharLambdaWavelength (Angstrom)0.1nmem.wlfloatEPLine excitation energy of lower leveleVphys.atmol.excitation;phys.atmol.level;spect.linefloatlog(gf)Log gf (oscillator strength)phys.absorption.coeff;arith.zpfloatf6Enhancement factor of classical van der Waals damping Gamma_6arith.factor;phys.dampingfloatg(upper)Statistical weight of upper level of linestat.weight;stat.maxintW(22879)? Equivalent width (milliAngstrom) for HD228790.1pmspect.line.eqWidthfloatnullableW(76932)? Equivalent width (milliAngstrom) for HD769320.1pmspect.line.eqWidthfloatnullableJ/A+A/326/751/tablea4Equivalent widths for the 30 programme starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElementChemical element and ionization stagephys.atmol.ionStage;phys.atmol.ionizationcharLambdaWavelength (Angstrom)0.1nmem.wlfloatEW(1)? Equivalent width (mA) for HD35670.1pmspect.line.eqWidthintnullableEW(2)? Equivalent width (mA) for CD-61 02820.1pmspect.line.eqWidthintnullableEW(3)? Equivalent width (mA) for HD172880.1pmspect.line.eqWidthintnullableEW(4)? Equivalent width (mA) for HD178200.1pmspect.line.eqWidthintnullableEW(5)? Equivalent width (mA) for G005-0400.1pmspect.line.eqWidthintnullableEW(6)? Equivalent width (mA) for CD-47 10870.1pmspect.line.eqWidthintnullableEW(7)? Equivalent width (mA) for HD228790.1pmspect.line.eqWidthintnullableEW(8)? Equivalent width (mA) for HD243390.1pmspect.line.eqWidthintnullableEW(9)? Equivalent width (mA) for HD257040.1pmspect.line.eqWidthintnullableEW(10)? Equivalent width (mA) for HD2412530.1pmspect.line.eqWidthintnullableEW(11)? Equivalent width (mA) for G102-0200.1pmspect.line.eqWidthintnullableEW(12)? Equivalent width (mA) for CD-33 33370.1pmspect.line.eqWidthintnullableEW(13)? Equivalent width (mA) for CD-57 16330.1pmspect.line.eqWidthintnullableEW(14)? Equivalent width (mA) for CD-45 32830.1pmspect.line.eqWidthintnullableEW(15)? Equivalent width (mA) for G088-0400.1pmspect.line.eqWidthintnullableEW(16)? Equivalent width (mA) for HD769320.1pmspect.line.eqWidthintnullableEW(17)? Equivalent width (mA) for G046-0310.1pmspect.line.eqWidthintnullableEW(18)? Equivalent width (mA) for HD832200.1pmspect.line.eqWidthintnullableEW(19)? Equivalent width (mA) for BD-21 34200.1pmspect.line.eqWidthintnullableEW(20)? Equivalent width (mA) for HD1037230.1pmspect.line.eqWidthintnullableEW(21)? Equivalent width (mA) for HD1050040.1pmspect.line.eqWidthintnullableEW(22)? Equivalent width (mA) for HD1060380.1pmspect.line.eqWidthintnullableEW(23)? Equivalent width (mA) for HD1065160.1pmspect.line.eqWidthintnullableEW(24)? Equivalent width (mA) for W75470.1pmspect.line.eqWidthintnullableEW(25)? Equivalent width (mA) for HD113083A0.1pmspect.line.eqWidthintnullableEW(26)? Equivalent width (mA) for HD113083B0.1pmspect.line.eqWidthintnullableEW(27)? Equivalent width (mA) for HD1136790.1pmspect.line.eqWidthintnullableEW(28)? Equivalent width (mA) for HD1205590.1pmspect.line.eqWidthintnullableEW(29)? Equivalent width (mA) for HD1210040.1pmspect.line.eqWidthintnullableEW(30)? Equivalent width (mA) for HD1266810.1pmspect.line.eqWidthintnullableJ/A+A/326/751/tablea5Abundance ratios and kinematical parametersNameDesignation of starmeta.id;meta.mainchareOrbital eccentricitysrc.orbital.eccentricitydoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintm_Name[AB] Multiplicity index on Namemeta.code.multipcharTeffEffective temperatureKphys.temperature.effectiveintlog(g)Logarithmic surface gravitylog(cm.s**-2)phys.gravityfloat[Fe/H]iron-to-hydrogen ratiolog(Sun)phys.abund.Fefloat[O/Fe]Oxygen-to-iron ratiolog(Sun)phys.abundfloat[Mg/Fe]Magnesium-to-iron ratiolog(Sun)phys.abundfloat[Si/Fe]Silicon-to-iron ratiolog(Sun)phys.abundfloat[Ca/Fe]Calcium-to-iron ratiolog(Sun)phys.abundfloat[Ti/Fe]Titanium-to-iron ratiolog(Sun)phys.abundfloat[Cr/Fe]Chromium-to-iron ratiolog(Sun)phys.abundfloat[Ni/Fe]Nickel-to-iron ratiolog(Sun)phys.abundfloat[Na/Fe]Sodium-to-iron ratiolog(Sun)phys.abundfloat[Y/Fe]Yttrium-to-iron ratiolog(Sun)phys.abundfloat[Ba/Fe]Barium-to-iron ratiolog(Sun)phys.abundfloatUvelGalactic U-velocity component relative LSRkm/sphys.veloc;pos.cartesian.x;pos.lsrdoubleVvelGalactic V-velocity component relative LSRkm/sphys.veloc;pos.cartesian.y;pos.lsrdoubleWvelGalactic W-velocity component relative LSRkm/sphys.veloc;pos.cartesian.z;pos.lsrdoubleV(tot)Total velocity relative to galactic centerkm/sphys.velocdoubleH(z)Angular momentum about z-axis of the Galaxykpc.km/sphys.angMomentumdoublez(max)Maximum value of z-coordinatekpcpos.distance;src.orbitalfloatR(max)Maximum distance from galactic centerkpcpos.distance;src.orbitalfloatz(min)Minimum value of z-coordinatekpcpos.distance;src.orbitaldoubleR(min)Minimum distance from galactic centerkpcpos.distance;src.orbitalfloat|z|(max)Maximum distance from the galactic planekpcpos.distance;src.orbitalfloat