J/MNRAS/316/514ivo://CDS.VizieR/J/MNRAS/316/514doi:10.26093/cds/vizier.73160514CDSAdelman S.J.Caliskan H.Kocer D.Hamami I.Tektunali H.G.2024-06-26T20:16:36Z2000-10-04T17:44:57ZCDS support team

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

cds-question@unistra.frchemically-peculiar-starsline-intensitiesElemental abundances of 28 And (A7III) and 99 Her (F7V), which have modest rotational velocities, are derived in a manner consistent with previous studies in this series of papers. The values for 28 And, a δ Scuti variable, show that it is slightly metal-poor, but not a classical Am star. 99 Her, which is somewhat more metal-poor, has a rather small microturbulence for its spectral type.2000MNRAS.316..514Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/316/514CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/107/353 : CP stars (Lopez-Garcia+, 1994)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+AS/137/227 : HD 133029 & HD 192913 abundances (Lopez-Garcia+ 1999)J/A+A/367/597 : ups Her, phi Her & HR 7018 abundances (Adelman+, 2001)J/A+A/367/859 : {alpha} Scl and HD 170973 abundances (Lopez-Garcia+, 2001)J/A+A/371/1078 : alpha Dra, tau Her, gamma Lyr, HR 7926 (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/MNRAS/316/514https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/316/514http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/316/514https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/316/514https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/316/514http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/316/514GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/MNRAS/316/514/table4aElemental abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIonIonphys.atmol.ionizationcharprimaryNoMultiplet number from Moore (1945) if first line of multiplet, if not from Moore an initial indicating the paper (1)phys.atmol.levelcharLambdaLaboratory wavelength (air)0.1nmem.wl;phys.atmol.transitionfloatlog(gf)Oscillator strengthphys.atmol.wOscStrengthfloatr_log(gf)Reference to oscillator strength (2)meta.refcharEW1? Equivalent width for 28 Andpmspect.line.eqWidthfloatnullablelog(N/Ntot)1? Elemental abundance for 28 And (3)phys.abundfloatnullableEW2? Equivalent width for 99 Herpmspect.line.eqWidthfloatnullablelog(N/Ntot)2? Elemental abundance for 99 Her (3)phys.abundfloatnullableJ/MNRAS/316/514/table4bRelative abundanceslog(El/Ntot)1? Elemental abundance for 28 And (1)phys.abundfloatnullablee_log(El/Ntot)1? rms uncertainty on log(El/Ntot)1stat.errorfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIonIonphys.atmol.ionizationcharprimaryElElementphys.atmol.elementcharlog(El/Ntot)2? Elemental abundance for 99 Her (1)phys.abundfloatnullablee_log(El/Ntot)2? rms uncertainty on log(El/Ntot)2stat.errorfloatnullable