Properties and nature of Be stars. XXII. Long-term light and spectral variations of the new bright Be star HD 6226

Photometric and spectroscopic monitoring of the B star HD 6226 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 mak...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2004-03, Vol.416 (2), p.669-676
Hauptverfasser: BOZIC, H, HARMANEC, P, BUIL, C, YANG, S, ZIZNOVSKY, J, PERCY, J. R, RUZDJAK, D, SUDAR, D, SLECHTA, M, SKODA, P, KRPATA, J
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Sprache:eng
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