Transient Corotating Clumps around Adolescent Low-mass Stars from Four Years of TESS

Transient Corotating Clumps around Adolescent Low-mass Stars from Four Years of TESS

Complex periodic variables (CPVs) are stars that exhibit highly structured and periodic optical light curves. Previous studies have indicated that these stars are typically disk-free pre-main-sequence M dwarfs with rotation periods ranging from 0.2 to 2 days. To advance our understanding of these en...

Full description

Bibliographic Details
Main Authors: Luke G. Bouma, Rahul Jayaraman, Saul Rappaport, Luisa M. Rebull, Lynne A. Hillenbrand, Joshua N. Winn, Alexandre David-Uraz, Gáspár Á. Bakos
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astronomical Journal
Subjects:
Weak-line T Tauri stars
Periodic variable stars
Circumstellar matter
Star clusters
Stellar magnetic fields
Stellar rotation
Online Access:https://doi.org/10.3847/1538-3881/ad0c4c

Internet

https://doi.org/10.3847/1538-3881/ad0c4c

Similar Items