J/ApJ/416/787ivo://CDS.VizieR/J/ApJ/416/787doi:10.26093/cds/vizier.14160787CDSSOON W.H.ZHANG Q.BALIUNAS S.L.KURUCZ R.L.1999-03-02T09:10:41Z1999-03-02T10:10:34ZCDS support team

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

cds-question@unistra.frgiant-starssupergiant-starsphotometrymetallicity(no description available)1993ApJ...416..787Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/416/787CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/416/787https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/416/787http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/416/787https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/416/787https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/416/787http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/416/787GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/ApJ/416/787/table1Data for dwarfsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHD[]? HD designationmeta.id;meta.mainintnullablem_HDMultiplicity index on HD designationmeta.code.multipcharn_HD[*] Note for HD 36389 (1)meta.notecharNameOther namemeta.idchar<Crv>[]? Time averaged spectrophotometric index Crv = 2.5 log (N_R/N_V) (2)magphot.colorfloatnullableo_<Crv>[]? Number of observed pointsmeta.numberintnullablee_<Crv>[]? Standard deviation of observed pointsmagstat.errorfloatnullableb-yObserved b-y indexmagphot.color;em.opt.B;em.opt.Vfloatm1Observed m1 indexmagphot.colorfloatc1[]? Observed c1 indexmagphot.colorfloatnullableV-K[]? Observed V-K indexmagphot.color;em.opt.V;em.IR.KfloatnullableTHETAeff[]? Observed stellar effective temperature (THETAeff= 5040/Teff, Teff in K)phys.temperature.effectivefloatnullablelog(g)[]? Observed surface gravitylog(cm.s**-2)phys.gravityfloatnullable[Fe/H]1[]? Scaled iron abundancephys.abund.Fefloatnullable[Fe/H]2[]? Highest value of metallicity when n_[Fe/H] = ,phys.abund.FefloatnullableDm[]? magnitude difference of the two components for double starsmagphot.mag;arith.difffloatnullableSep[]? Maximum observed separation for double starsarcsecpos.angDistancefloatnullablePeriodOrbital period for double stars The symbols SBa and SB identify the primary star associated with a known or suspected spectroscopic binary system.time.periodcharJ/ApJ/416/787/table2Data for giantsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHD[]? HD designationmeta.idintnullablem_HDMultiplicity index on HD designationmeta.code.multipcharn_HD[*] Note for HD 36389 (1)meta.notecharNameOther namemeta.idchar<Crv>[]? Time averaged spectrophotometric index Crv = 2.5 log (N_R/N_V) (2)magphot.colorfloatnullableo_<Crv>[]? Number of observed pointsmeta.numberintnullablee_<Crv>[]? Standard deviation of observed pointsmagstat.errorfloatnullableb-yObserved b-y indexmagphot.color;em.opt.B;em.opt.Vfloatm1Observed m1 indexmagphot.colorfloatc1[]? Observed c1 indexmagphot.colorfloatnullableV-K[]? Observed V-K indexmagphot.color;em.opt.V;em.IR.KfloatnullableTHETAeff[]? Observed stellar effective temperature (THETAeff= 5040/Teff, Teff in K)phys.temperature.effectivefloatnullablelog(g)[]? Observed surface gravitylog(cm.s**-2)phys.gravityfloatnullable[Fe/H]1[]? Scaled iron abundancephys.abund.Fefloatnullable[Fe/H]2[]? Highest value of metallicity when n_[Fe/H] = ,phys.abund.FefloatnullableDm[]? magnitude difference of the two components for double starsmagphot.mag;arith.difffloatnullableSep[]? Maximum observed separation for double starsarcsecpos.angDistancefloatnullablePeriodOrbital period for double stars The symbols SBa and SB identify the primary star associated with a known or suspected spectroscopic binary system.time.periodchar