UBV photometry of HD 6226 (Bozic+, 2004)

Details UBV photometry of HD 6226 (Bozic+, 2004) UBV photometry of HD 6226 (Bozic+, 2004)

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ycat..34160669b&link_type=abstract

VizieR On-line Data Catalog: J/A+A/416/669. Originally published in: 2004A&A...416..669B

Physics

Stars: Emission, Binaries: Spectroscopic, Photometry: Ubv, Spectrophotometry

Scientific paper

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.
(3 data files).

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