This is a Be star showing emission features in its Balmer lines due to a circumstellar disk of decreated gas. It is classified as a suspected Gamma Cassiopeiae type variable star with a visual magnitude varying from +4.30 down to +4.39.
This is a Be star exhibiting emission in its Balmer lines caused by a circumstellar disk of disintegrated gas. It is categorized as a suspected Gamma Cassiopeiae type variable star with a visual magnitude fluctuating from +4.30 to +4.39.