Inactive Longitude and Superflare in the Active Single-lined Pre-main-sequence Binary V2279 Cyg

Inactive Longitude and Superflare in the Active Single-lined Pre-main-sequence Binary V2279 Cyg

Young, solar-like stars in the pre-main-sequence (PMS) stage exhibit vigorous magnetic activity that significantly influences their circumstellar environments and the processes of planetary formation and evolution. In binary systems, tidal forces and magnetic interactions can further shape the magne...

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Bibliographic Details
Main Authors: Xueying Hu, Tianqi Cang, Jian-Ning Fu, Xuan Wang, Keyu Xing, Haotian Wang, Pascal Petit, Jiaxin Wang, Yong Yang, He Zhao
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Flare stars
Binary stars
Pre-main sequence stars
Magnetic fields
Stellar activity
Online Access:https://doi.org/10.3847/1538-4357/adeb69
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https://doi.org/10.3847/1538-4357/adeb69

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