J/A+A/367/859ivo://CDS.VizieR/J/A+A/367/859doi:10.26093/cds/vizier.33670859CDSLopez-Garcia Z.Adelman S.J.Pintado O.I.2001-04-22T17:47:54Z2001-04-22T17:47:48ZCDS support team

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

cds-question@unistra.frpeculiar-variable-starschemically-peculiar-starsline-intensitiesFine analyses of the magnetic CP stars {alpha} Scl and HD 170973 are presented using ATLAS9 model atmospheres which have same bulk metallicity as the deduced abundances. The light elements are mostly solar except for silicon, and all the heavier elements except nickel in HD 170973, which is solar, are greatly overabundant. The iron peak elements are typically 10 times overabundant, Sr is of order of 1000 times solar, Y and Zr are of order of 100 times solar. The rare earths are 1000 or more times overabundant.2001A&A...367..859Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/367/859CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/107/353 : Paper I. HD 43819 and HD 147550 (Lopez-Garcia+, 1994)J/A+AS/137/227 : Paper II. HD 133029 and HD 192913 (Lopez-Garcia+, 1999)J/A+AS/125/219 : mu Lep, 7 Sex, HR 4817 & 28 Her abundances (Adelman+ 1997)J/A+AS/129/563 : Abundances of HR 4487, 14 Hyd and 3 Cen A (Pintado+ 1998)J/MNRAS/316/514 : 28 And + 99 Her elemental abundances (Adelman+, 2000)J/A+A/394/187 : {gamma} Ser & 101 Her elemental abundances (Caliskan+, 2002)J/A+A/406/975 : theta And, eps Del, eps Aqr, iota And (Kocer+, 2003)J/A+A/406/987 : xi Oct, alpha Sex, 68 Tau elemental abund. (Pintado+, 2003)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/367/859https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/367/859http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/367/859https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/367/859https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/367/859http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/367/859GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/367/859/table4aElemental abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIonIon designationphys.atmol.ionizationcharMultMultiplet number from Moore (1945) if first line of multipletphys.atmol.levelcharlambdaLaboratory wavelength (air)0.1nmem.wl;phys.atmol.transitiondoubleloggfOscillator strengthphys.atmol.wOscStrengthfloatr_loggfReference to oscillator strength (1)meta.refcharEW1? Equivalent width for HD 170973pmspect.line.eqWidthfloatnullablelog(N/Ntot)1? log N/N_T_ value for HD 170973phys.abundfloatnullableEW2? Equivalent width for {alpha} Sclpmspect.line.eqWidthfloatnullablelog(N/Ntot)2? log N/N_T_ value for {alpha} Sclphys.abundfloatnullableJ/A+A/367/859/table4bRelative abundancesElElementphys.atmol.elementcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIonIonphys.atmol.ionizationcharprimarylog(El/Ntot)1? Elemental abundance for HD 170973 (1)phys.abundfloatnullablee_log(El/Ntot)1? rms uncertainty on log(El/Ntot)1stat.errorfloatnullablelog(El/Ntot)2? Elemental abundance for {alpha} Scl (1)phys.abundfloatnullablee_log(El/Ntot)2? rms uncertainty on log(El/Ntot)2stat.errorfloatnullable