B-type Supergiants in the SMC

DOI

High-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.

Cone search capability for table J/A+A/434/1125/table1 (Observational summary of the nine program stars and AzV 304)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34341125
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/434/1125
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/434/1125
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/434/1125
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/434/1125
Provenance
Creator Dufton P.L.; Ryans R.S.I.; Trundle; C.; Lennon D.J.; Hubeny I.; Lanz T.,Allende Prieto C.
Publisher CDS
Publication Year 2005
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy