Simulated Coronal Mass Ejections on a Young Solar-type Star and the Associated Instantaneous Angular Momentum Loss

Simulated Coronal Mass Ejections on a Young Solar-type Star and the Associated Instantaneous Angular Momentum Loss

Coronal mass ejections (CMEs) on stars can change the stars’ magnetic field configurations and mass-loss rates during the eruption and propagation and therefore, may affect the stars’ rotation properties on long timescales. The dynamics of stellar CMEs and their influence on the stellar angular mome...

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Bibliographic Details
Main Authors: Yu Xu, Julián D. Alvarado-Gómez, Hui Tian, Katja Poppenhäger, Gustavo Guerrero, Xianyu Liu
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Stellar coronal mass ejections
Magnetohydrodynamical simulations
Stellar winds
Stellar mass loss
Stellar magnetic fields
Online Access:https://doi.org/10.3847/1538-4357/ad5845

Internet

https://doi.org/10.3847/1538-4357/ad5845

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