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What is Detecting Active Be Stars in Clusters about?

This article presents a new method for detecting and characterizing active Be star candidates in poorly studied young open clusters using data from Gaia DR2 and DR3. The authors test their methodology on four open clusters known for hosting Be stars and demonstrate that their approach can effectively identify candidates based on photometric variability. The findings suggest that extending this methodology to other clusters may increase the number of identified Be stars, enhancing our understanding of their

Author

chakrabortyarghya234

Language

EN