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

Abstract

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.

Keywords

• Properties
• nature
• stars
• Long-term
• light
• spectral
• variations
• bright
• 6226