UBV photometry of HD 6226 Virtual Observatory Resource

Authors

1. Bozic H.
2. Harmanec P.
3. Yang S.
4. Ziznovsky J.
5. Percy J.
6. Ruzdjak D.,Sudar D.
7. Slechta M.
8. Skoda P.
9. Krpata J.
10. Buil C.

Published by

CDS

Abstract

Photometric and spectroscopic monitoring of the B star resulted in the finding that this object is a new bright Be star with a clear positive correlation between the brightness and emission-line strength. The emission-line episodes are relatively short and seem to repeat frequently which makes this star an ideal target for studying the causes of the Be phenomenon.

Keywords

1. emission-line-stars
2. spectroscopic-binary-stars
3. visible-astronomy
4. Wide-band photometry
5. spectrophotometry

Bibliographic source Bibcode

2004A&A...416..669B

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/416/669

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/416/669

Document Object Identifer DOI

doi:10.26093/cds/vizier.34160669

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/416/669
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/416/669
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/416/669

IVOA Table Access TAP

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