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 |
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Sprache: | eng |
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