UBV photometry of HD 6226

DOI

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.

Identifier
DOI http://doi.org/10.26093/cds/vizier.34160669
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/416/669
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/416/669
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/416/669
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/416/669
Provenance
Creator Bozic H.; Harmanec P.; Yang S.; Ziznovsky J.; Percy J.; Ruzdjak D.,Sudar D.; Slechta M.; Skoda P.; Krpata J.; Buil C.
Publisher CDS
Publication Year 2004
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; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy