J/MNRAS/369/1677ivo://CDS.VizieR/J/MNRAS/369/1677doi:10.26093/cds/vizier.73691677CDSPandey G.Reddy B.E.2024-07-02T20:17:37Z2007-04-12T05:28:14ZCDS support team

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

cds-question@unistra.frvariable-starschemically-peculiar-starsAbundance analysis of the cool extreme helium (EHe) star LSS 3378 is presented. The abundance analysis is done using local thermodynamic equilibrium (LTE) line formation and LTE model atmospheres constructed for EHe stars.2006MNRAS.369.1677Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/369/1677CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/369/1677https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/369/1677http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/369/1677https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/369/1677https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/369/1677http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/369/1677GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/MNRAS/369/1677/tablea1Lines used to derive elemental abundances in LSS 3378recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIonIon (1)phys.atmol.ionStagecharLambdaWavelength of the line0.1nmem.wlfloatEPlowLower excitation potentialeVphys.atmol.excitation;stat.minfloatloggfOscillator strengthphys.atmol.oscStrengthfloatr_loggfloggf reference (3)meta.bibcharEW? Measured equivalent width0.1nmspect.line.eqWidthintnullablen_EW[S] S: Spectrum synthesismeta.notecharlogEpsIndividual elemental abundance (2)phys.abundfloat