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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Bibliografski detalji
Glavni autori: Mageshwaran Tamilan, Kimitake Hayasaki, Takeru K. Suzuki
Format: Članak
Jezik:English
Izdano: IOP Publishing 2024-01-01
Serija:The Astrophysical Journal
Teme:
Accretion
Tidal disruption
Magnetohydrodynamics
High energy astrophysics
Online pristup:https://doi.org/10.3847/1538-4357/ad7603

Internet

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

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