J/A+A/447/685ivo://CDS.VizieR/J/A+A/447/685doi:10.26093/cds/vizier.34470685CDSAdelman S.J.Caliskan H.Gulliver A.F.Teker A.2006-04-16T20:30:22Z2006-04-16T20:28:54ZCDS support team

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

cds-question@unistra.frpeculiar-variable-starschemically-peculiar-starsWe performed elemental abundances analyses of the mercury-manganese (HgMn) stars 53 Tau, {beta} Tau, and {gamma} Crv consistent with previous studies of similar stars in this series.2006A&A...447..685Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/447/685CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/354/899 : Elemental abundance analyses IV. (Adelman+, 2000)J/A+A/367/597 : ups Her, phi Her + HR 7018 (XXIV) (Adelman+, 2001)J/A+A/367/859 : {alpha} Scl and HD 170973 abundances (Lopez-Garcia+, 2001)J/A+A/371/1078 : Elemental abundance analyses XXV (Adelman+, 2001)J/A+A/394/187 : {gamma} Ser + 101 Her (XXVI) (Caliskan+, 2002)J/A+A/406/975 : Elemental abundance analyses XXVII (Kocer+, 2003)J/A+A/406/987 : Elemental abundances of three CP stars (Pintado+, 2003)J/A+AS/107/353 : CP stars (Lopez-Garcia+, 1994)J/A+AS/125/219 : mu Lep, 7 Sex, HR 4817 + 28 Her (Adelman+ 1997)J/A+AS/129/563 : Abundances of HR 4487, 14 Hyd and 3 Cen A (Pintado+ 1998)J/A+AS/137/227 : HD 133029 + HD 192913 (II)_ (Lopez-Garcia+ 1999)J/MNRAS/316/514 : 28 And + 99 Her (XXIII) (Adelman+, 2000)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/447/685https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/447/685http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/447/685https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/447/685https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/447/685http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/447/685GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/447/685/abundAtomic abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namemeta.id;meta.maincharIonIonphys.atmol.ionStagecharElementElement (identical to bytes 11-12)phys.atmol.elementcharlog(Nel/Ntot)Derived abundance of element (1)phys.atmol.elementfloate_log(Nel/Ntot)? rms uncertainty on logEl/NTstat.errorfloatnullableJ/A+A/447/685/table4He/H determinationsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namemeta.id;meta.maincharlambdaWavelength0.1nmem.wlintHe/HHe/H abundace value (1)phys.abund.YfloatJ/A+A/447/685/tab567Abundances for {beta} Tau, {gamma} Crv, 53 Tau and from newly measured lines of {upsilon} HerrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namemeta.id;meta.maincharIonIonphys.atmol.ionStagecharMultMultiplet number (1)meta.idcharlambdaLaboratory wavelength0.1nmem.wlfloatlog(gf)log gf valuephys.absorption.coeff;arith.zpfloatr_log(gf)Reference for log(gf) (2)meta.bibcharEWlambda? Equivalent width0.1pmspect.line.eqWidthintnullablelog(Nel/Ntot)? Derived abundancephys.abundfloatnullableJ/A+A/447/685/table8Comparison of Results (logN/H) for 53 Tau, {gamma} Crv, and {upsilon} Her last analysis with this paperNameStar namemeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIonIonphys.atmol.ionStagecharlog(Nel/H)oldPrevious relative abundance (1)phys.abundfloatlog(Nel/H)This Paper relative abundancephys.abundfloat