J/A+AS/141/491ivo://CDS.VizieR/J/A+AS/141/491CDSChen Y.QNissen P.E.Zhao G.Zhang H.W.Benoni T.2017-12-15T10:54:51Z2004-11-21T21:29:39ZCDS support team

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

cds-question@unistra.frdwarf-starschemically-peculiar-starsline-intensitiesTable 3. Atmospheric parameters, space velocities, distances, masses and ages of the program stars. Table 4. Atomic line data including wavelength, excitation energy of the lower level, the logarithm of the oscillator strength (the experimental or theoretical value, the corrected value and the differential value from standard stars) and the adopted enhancement factor of the Unsold approximation to the van der Waals damping constant. The last column gives the equivalent width in the spectrum of HD 142373 representing a typical metallicity of the sample of stars. Uncertain EWs marked by (:) and strong lines with EW>100m{AA} are not used in the abundance determination for this star. Table 5. Abundance ratios for the program stars. The oxygen abundance is derived from the 7774{AA} triplet but scaled to results from the forbidden [OI] line at 6300{AA}.2000A&AS..141..491Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/141/491CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/141/491https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/141/491http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/141/491https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/141/491https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/141/491http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/141/491GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+AS/141/491/table3 (Stellar atmospheric parameters, space velocities, distances, masses and ages)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+AS/141/491/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/A+AS/141/491/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+AS/141/491/table3?GETtext/xml+votable180.050000true2.17057636.6271250.0055555555555555566/1330 1341 1603 1788 2169 2234 2476 2637 2771 3102 3741 3913 4227 4491 4854 4895 5065 5088 5154 5522 6066 6153 6165 6326 6539 6761 6926 6941 7115 7390 7505 8279 8476 8746 8995 9435 9835 9841 10247 10375 10972 11314 11732 11858 12295 12512 12592 12704 13440 13478 13943 14001 14180 15030 15910 16105 16338 18289 18615 19217 20446 21696 21699 22518 22868 23140 23190 23796 23938 24151 24160 25435 25444 26110 26521 26676 26748 27006 27075 27831 28180 29784 31029 31132 32473 32612 40679 48613 48883 48967https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+AS/141/491?format=asciiOpticaldefaultJ/A+AS/141/491/table3Stellar atmospheric parameters, space velocities, distances, masses and agesUvelGalactic U velocity (1)km/sphys.velocfloatVvelGalactic V velocity (1)km/sphys.velocfloatWvelGalactic W velocity (1)km/sphys.velocfloatDistHeliocentric Distancepcpos.distancefloatMassStellar masssolMassphys.massfloatAgeStellar ageGyrtime.agefloatu_Age[:] indicates uncertain agemeta.code.errorcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHDHD <Cat. <III/135>) number of the starmeta.id;meta.maincharf_HD[BV] B: suspected binary, V: variablemeta.code.errorcharT(eff)Effective temperatureKphys.temperature.effectivefloatlog(g)Logarithmic surface gravitycm.s**-2phys.gravityfloat[Fe/H]Iron-to-hydrogen ratiolog(Sun)phys.abund.FefloatVturbMicroturbulence velocitykm/sphys.veloc.microTurbfloatSimbadSimbad column added by the CDSmeta.refchar_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+AS/141/491/table4Atomic line data and equivalent widths for HD 142373recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElementChemical element and ionization stagephys.atmol.elementcharLambdaWavelength0.1nmem.wldoubleEPLine excitation energy of lower leveleVphys.energy;phys.atmol.excitationfloatlog(gf)t? Experimental or theoretical log(gf) valuephys.atmol.wOscStrengthfloatnullablelog(gf)c? Corrected log(gf) valuephys.atmol.wOscStrengthfloatnullablelog(gf)d? Differencial log(gf) value from standard starsphys.atmol.wOscStrengthfloatnullableE6Enhancement factor of the Unsold approximation to the van der Waals damping constantphys.damping;phys.atmolfloatEW? Equivalent width for HD 1423730.1pmspect.line.eqWidthfloatnullableu_EW[:] indicates uncertain equivalent widthmeta.code.errorcharJ/A+AS/141/491/table5Abundance ratiosrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHDHD (Cat. <III/135>) number of starmeta.id;meta.mainchar[Fe/H]IIron-to-hydrogen ratio from FeI lineslog(Sun)phys.abund.Fefloat[Fe/H]IIIron-to-hydrogen ratio from FeII lineslog(Sun)phys.abund.Fefloat[O/Fe]? Oxygen-to-iron ratiolog(Sun)phys.abundfloatnullable[Na/Fe]? Sodium-to-iron ratiolog(Sun)phys.abundfloatnullable[Mg/Fe]? Magnesium-to-iron ratiolog(Sun)phys.abundfloatnullable[Al/Fe]? Aluminium-to-iron ratiolog(Sun)phys.abundfloatnullable[Si/Fe]? Silicon-to-iron ratiolog(Sun)phys.abundfloatnullable[K/Fe]? Potassium-to-iron ratiolog(Sun)phys.abundfloatnullable[Ca/Fe]? Calcium-to-iron ratiolog(Sun)phys.abundfloatnullable[Ti/Fe]? Titanium-to-iron ratiolog(Sun)phys.abundfloatnullable[V/Fe]? Vanadium-to-iron ratiolog(Sun)phys.abundfloatnullable[Cr/Fe]? Chromium-to-iron ratiolog(Sun)phys.abundfloatnullable[Ni/Fe]? Nickel-to-iron ratiolog(Sun)phys.abundfloatnullable[Ba/Fe]? Barium-to-iron ratiolog(Sun)phys.abundfloatnullable