J/A+A/354/899ivo://CDS.VizieR/J/A+A/354/899doi:10.26093/cds/vizier.33540899CDSAdelman S.J.Pintado O.I.2024-08-06T20:00:26Z2000-04-01T10:17:19ZCDS support team

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

cds-question@unistra.frpeculiar-variable-starschemically-peculiar-starsUsing new CASLEO echelle spectrograms, we extended our elemental abundances of the sharp-lines Mercury-Manganese star {mu} Lep, 14 Hya, {kappa} Cnc, HR 4487, 28 Her, and HR 7245, the closely related star 3 CenA, and 7 Sex an A0V star with population I abundances, but with Population II star space motion. The {lambda}{lambda}4500-6200 region contains a sufficient number of lines to derive high-quality abundances of these stars. For most stars, the new spectra provide additional lines for the analyses which improve their quality as well as help fill in the periodic table.2000A&A...354..899Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/354/899CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/125/219 : Paper II. (mu Lep, 7 Sex, HR 4817, 28 Her) (Adelman+ 1997)J/A+AS/129/563 : Paper III. (HR 4487, 14 Hyd and 3 Cen A) (Pintado+ 1998)J/A+AS/107/353 : CP stars (Lopez-Garcia+, 1994)J/A+AS/137/227 : HD 133029 & HD 192913 abundances (Lopez-Garcia+ 1999)J/MNRAS/316/514 : 28 And & 99 Her elemental abundances (Adelman+, 2000)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/354/899https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/354/899http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/354/899https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/354/899https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/354/899http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/354/899GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/354/899/abundAtomic abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namemeta.id;meta.maincharprimaryIonIonphys.atmol.ionStagecharNlineNumber of linesmeta.numberintElementElement (identical to bytes 14-15)phys.atmol.elementcharlog(Nel/Ntot)Derived abundance of Element (ratio of number of atoms to the total number of atoms per unit volume)phys.atmol.elementfloate_log(Nel/Ntot)? rms uncertainty on log(Nel/Ntot)stat.errorfloatnullableJ/A+A/354/899/table5Elemental abundancesNameStar namemeta.id;meta.maincharprimaryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIonIonphys.atmol.ionStagecharMult? Multiplet numbermeta.idcharlambdaWavelength0.1nmem.wlfloatlog(gf)Oscillator strengthphys.atmol.oscStrengthfloatr_log(gf)Reference for log(gf) (1)meta.ref;pos.framecharEW? Equivalent width0.0001nmspect.line.eqWidthintnullablelog(N/Ntot)Derived abundance in relative number of atoms per unit volumephys.abundfloat