Identification of Possible Stellar Companions via Speckle Interferometry in a Sample of Be Stars II

This study investigates the identification of possible stellar companions in a sample of Be stars using speckle interferometry. Be stars, which are rapidly rotating B-type stars exhibiting emission lines due to the presence of circumstellar disks, have been proposed to potentially reside in binary o...

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Bibliographic Details
Main Authors: C. A. Guerrero, T. B. Souza, M. Borges Fernandes, A. D. Guajardo Jurado
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astronomical Journal
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Online Access:https://doi.org/10.3847/1538-3881/adbf11
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