J/A+A/434/1125ivo://CDS.VizieR/J/A+A/434/1125doi:10.26093/cds/vizier.34341125CDSDufton P.L.Ryans R.S.I.TrundleC.Lennon D.J.Hubeny I.Lanz T.,Allende Prieto C.2005-05-22T16:18:01Z2005-05-22T16:17:54ZCDS support team

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

cds-question@unistra.frsupergiant-starsb-starsline-intensitiesHigh-resolution UCLES/AAT spectra are presented for nine B-type supergiants in the SMC, chosen on the basis that they may show varying amounts of nuclear-synthetically processed material mixed to their surface. These spectra have been analysed using a new grid of approximately 12000 non-LTE line blanketed TLUSTY model atmospheres to estimate atmospheric parameters and chemical composition.2005A&A...434.1125Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/434/1125CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/304/347 : 40 field red supergiants in the SMC (Meliani+, 1995)J/A+A/324/435 : Chemical composition of 6 K supergiants in the SMC (Hill, 1997)J/A+AS/30/261 : UBV and Radial Velocities of SMC Supergiants (Ardeberg+, 1977)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/434/1125https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/434/1125http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/434/1125https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/434/1125https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/434/1125http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/434/1125GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/434/1125/table1 (Observational summary of the nine program stars and AzV 304)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/434/1125/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/434/1125/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/434/1125/table1?GETtext/xml+votable180.050000true12.66-73.4716670.0055555555555555566/32958 33295 33298 33304 33306 33328https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/434/1125?format=asciiOpticaldefaultJ/A+A/434/1125/table1Observational summary of the nine program stars and AzV 304recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namecharprimaryRAJ2000Right ascension (J2000.0), from Simbadpos.eq.ra;meta.mainDEJ2000Declination (J2000.0), from Simbadpos.eq.dec;meta.mainVmagVisual V magnitudemagfloatSpTypeMK spectral typecharS/N? Signal-to-noise ratiointnullableHRV? Heliocentric radial velocitykm/sintnullableFWHM? FWHM of the metal absorption line spectrumkm/sintnullableJ/A+A/434/1125/table4Equivalent Widths Measurements and line-by-line abundances for SMC supergiants and AzV 304recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameStar namecharSpecIonic species of the elementcharLambdaRest wavelength of the spectral line0.1nmfloatn_Lambda[B] B: the feature is a close doubletcharExcExcitation of the lower level of the transition For close doublets the mean value is giveneVfloatloggfLogarithm of the oscillator strength times degeneracy of the lower level. For doublets the value is the sum of the componentsfloatEWEquivalent width of the star spectral linespmfloatAbundAbundance estimate (1)float