Evolution of Tidal Disruption Event Disks with Magnetically Driven Winds

Evolution of Tidal Disruption Event Disks with Magnetically Driven Winds

We present a time-dependent, one-dimensional, magnetically driven disk wind model based on magnetohydrodynamic (MHD) equations, in the context of tidal disruption events (TDEs). We assume that the disk is geometrically thin, is gas pressure dominated, and explicitly accounts for magnetic braking and...

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Bibliographic Details
Main Authors: Mageshwaran Tamilan, Kimitake Hayasaki, Takeru K. Suzuki
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Accretion
Tidal disruption
Magnetohydrodynamics
High energy astrophysics
Online Access:https://doi.org/10.3847/1538-4357/ad7603

Internet

https://doi.org/10.3847/1538-4357/ad7603

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