J/A+AS/137/227ivo://CDS.VizieR/J/A+AS/137/227CDSLopez-Garica Z.Adelman S.J.1999-06-19T18:04:18Z1999-06-19T18:03:48ZCDS 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 silicon stars HD 133029 and HD 192913 are presented using ATLAS9 model atmospheres whose predictions fit the optical region spectrophotometry and H{gamma} profiles and have the same bulk metallicity as the deduced abundances. Both are very He poor stars. The light elements are mostly solar except for silicon, and all the heavier elements, except nickel in HD 133029 which is solar, are greatly overabundant. The iron peak elements are typically 10 times overabundant. SrYZr are of order of 100 times solar. The rare earths are 1000 or more times overabundant.1999A&AS..137..227Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/137/227CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/107/353 : Paper I. HD 43819, HD 147550 (Lopez-Garcia+, 1994)J/A+A/367/859 : Paper III. {alpha} Scl and HD 170973 (Lopez-Garcia+, 2001)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/A+A/354/899 : Elemental abundance analyses. IV. (Adelman+, 2000)J/MNRAS/316/514 : 28 And & 99 Her elemental abundances (Adelman+, 2000)J/A+A/367/597 : ups Her, phi Her & HR 7018 abundances (Adelman+, 2001)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+AS/137/227https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/137/227http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/137/227https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/137/227https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/137/227http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/137/227GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+AS/137/227/table4aElemental abundancesElElementphys.atmol.elementcharprimaryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNo? Multiplet Numberphys.atmol.levelintnullableLambdaWavelength0.1nmem.wldoublelog(gf)Oscillator strengthphys.atmol.wOscStrengthfloatr_log(gf)Reference to oscillator strength (1)meta.refcharW1? Equivalent width for HD 133029pmspect.line.eqWidthfloatnullablelog(N/Ntot)1? Deduced abundance for HD 133029 (2)phys.abundfloatnullableW2? Equivalent width for HD 192913pmspect.line.eqWidthfloatnullablelog(N/Ntot)2? Deduced abundance for HD 192913 (2)phys.abundfloatnullableJ/A+AS/137/227/table4bRelative abundancesElElementphys.atmol.elementcharprimaryrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlog(El/Ntot)1? Elemental abundance for HD 133029 (1)phys.abundfloatnullablee_log(El/Ntot)1? rms uncertainty on log(El/Ntot)1stat.errorfloatnullablelog(El/Ntot)2? Elemental abundance for HD 192913 (1)phys.abundfloatnullablee_log(El/Ntot)2? rms uncertainty on log(El/Ntot)2stat.errorfloatnullable