Bulk Motions in the Black Hole Jet Sheath as a Candidate for the Comptonizing Corona

Bulk Motions in the Black Hole Jet Sheath as a Candidate for the Comptonizing Corona

Using two-dimensional general relativistic resistive magnetohydrodynamic simulations, we investigate the properties of the sheath separating the black hole jet from the surrounding medium. We find that the electromagnetic power flowing through the jet sheath is comparable to the overall accretion po...

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Bibliographic Details
Main Authors: Navin Sridhar, Bart Ripperda, Lorenzo Sironi, Jordy Davelaar, Andrei M. Beloborodov
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Black hole physics
High energy astrophysics
Magnetohydrodynamical simulations
Plasma astrophysics
X-ray binary stars
X-ray active galactic nuclei
Online Access:https://doi.org/10.3847/1538-4357/ada385
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https://doi.org/10.3847/1538-4357/ada385

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