Bright Be shell stars Virtual Observatory Resource

Authors

1. Rivnius T.
2. Baade D.
3. Stefl S.

Published by

CDS

Abstract

Echelle observations are presented and discussed for 23 of the 27 known "normal" shell stars brighter than about 6.5mag. In addition to those typical cases, three stars with known transitions between emission & shell and pure emission line appearance, and three rapidly rotating B stars without records of line emission (Bn stars) are added to the sample.

Keywords

1. be-stars
2. emission-line-stars
3. spectroscopy

Bibliographic source Bibcode

2006A&A...459..137R

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/459/137

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/459/137

Document Object Identifer DOI

doi:10.26093/cds/vizier.34590137

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/459/137
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/459/137
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/459/137

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).