J/A+A/293/347ivo://CDS.VizieR/J/A+A/293/347doi:10.26093/cds/vizier.32930347CDSHILL V.ANDRIEVSKY S.SPITE M.1997-12-09T16:25:21Z1997-12-09T17:25:17ZCDS support team

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

cds-question@unistra.frmagellanic-cloudssupergiant-starsspectroscopychemical-abundances(no description available)1995A&A...293..347Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/293/347CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/293/347https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/293/347http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/293/347https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/293/347https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/293/347http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/293/347GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/293/347/appendixLines used in the analysis, with their equivalent width and individual abundance for each of the nine investigated LMC supergiants and for Canopus.recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLambdaCentral wavelength of the line0.1nmem.wlfloatEl.Name of the elementphys.atmol.elementcharEl.Ion.Degree of ionization of the element (1 for neutral and 2 for ionized species)phys.atmol.ionizationintXi(ex)Excitation potential of the lineeVphys.energy;phys.atmol.excitationfloatlog(gf)Line transition probability in log scalephys.atmol.wOscStrengthfloatWG244[]? Equivalent width of the line for star G2440.1nmspect.line.eqWidthfloatn_AG244[* ] Note on the abundance determination (1)meta.notecharAG244[]? Abundance normalised to the Sun for G244Sunphys.abundfloatWG258[]? Equivalent Width of the line for star G2580.1nmspect.line.eqWidthfloatn_AG258[* ] Note on the abundance determination (1)meta.notecharAG258[]? Abundance normalised to the Sun for G258Sunphys.abundfloatWG274[]? Equivalent Width of the line for star G2740.1nmspect.line.eqWidthfloatn_AG274[* ] Note on the abundance determination (1)meta.notecharAG274[]? Abundance normalised to the Sun for G274Sunphys.abundfloatWG319[]? Equivalent Width of the line for star G3190.1nmspect.line.eqWidthfloatn_AG319[* ] Note on the abundance determination (1)meta.notecharAG319[]? Abundance normalised to the Sun for G319Sunphys.abundfloatWG396[]? Equivalent Width of the line for star G3960.1nmspect.line.eqWidthfloatn_AG396[* ] Note on the abundance determination (1)meta.notecharAG396[]? Abundance normalised to the Sun for G396Sunphys.abundfloatWG406[]? Equivalent Width of the line for star G4060.1nmspect.line.eqWidthfloatn_AG406[* ] Note on the abundance determination (1)meta.notecharAG406[]? Abundance normalised to the Sun for G406Sunphys.abundfloatWG439[]? Equivalent Width of the line for star G4390.1nmspect.line.eqWidthfloatn_AG439[* ] Note on the abundance determination (1)meta.notecharAG439[]? Abundance normalised to the Sun for G439Sunphys.abundfloatWG501[]? Equivalent Width of the line for star G5010.1nmspect.line.eqWidthfloatn_AG501[* ] Note on the abundance determination (1)meta.notecharAG501[]? Abundance normalised to the Sun for G501Sunphys.abundfloatWG538[]? Equivalent Width of the line for star G5380.1nmspect.line.eqWidthfloatn_AG538[* ] Note on the abundance determination (1)meta.notecharAG538[]? Abundance normalised to the Sun for G538Sunphys.abundfloatWCan[]? Equivalent Width of the line for Canopus (taken from Luck & Lambert, 1985 and Desikachary & Hearnshaw, 1982)0.1nmspect.line.eqWidthfloatn_ACan[*# ] Note on the abundance determination (1)meta.notecharACan[]? Abundance normalised to the Sun for CanopusSunphys.abundfloat