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Inverse Compton Emission and Cooling of Relativistic Particles Accelerated at Shear Boundary Layers in Relativistic Jets

Both observational evidence and theoretical considerations from magnetohydrodynamic simulations of jets suggest that the relativistic jets of active galactic nuclei (AGN) are radially stratified, with a fast inner spine surrounded by a slower-moving outer sheath. The resulting relativistic shear lay...

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Détails bibliographiques
Auteurs principaux: Tej Chand, Markus Böttcher
Format: Artigo
Langue:Inglês
Publié: IOP Publishing 2024-01-01
Collection:The Astrophysical Journal
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Accès en ligne:https://doi.org/10.3847/1538-4357/ad0a63
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