Three-dimensional Simulations of Magnetospheric Accretion in a T Tauri Star: Accretion and Wind Structures Just Around the Star

We perform three-dimensional (3D) magnetohydrodynamic simulations of magnetospheric accretion in a T Tauri star to study the accretion and wind structures in the close vicinity of the star. The gas accreting onto the star consists of the gas from the magnetospheric boundary and the failed disk winds...

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Bibliographic Details

Published in:	The Astrophysical Journal
Main Authors:	Shinsuke Takasao, Kengo Tomida, Kazunari Iwasaki, Takeru K. Suzuki
Format:	Article
Language:	English
Published:	IOP Publishing 2022-01-01
Subjects:	Pre-main sequence stars Star formation Magnetohydrodynamical simulations Stellar magnetic fields Stellar accretion disks Protostars
Online Access:	https://doi.org/10.3847/1538-4357/ac9eb1