Magnetic Pressure Dominance Stabilizes AGN Disks against Gravitational Instability

Magnetic effects have long been considered a possible factor in stabilizing the outer regions of active galactic nuclei accretion disks against gravitational instability (GI). However, the computational demands of testing this hypothesis have prevented comprehensive study of this problem. Here, we p...

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Detalles Bibliográficos

Autores principales:	Hannalore J. Gerling-Dunsmore, Mitchell C. Begelman, Jacob B. Simon, Philip J. Armitage
Formato:	Artigo
Lenguaje:	Inglês
Publicado:	IOP Publishing 2026-01-01
Colección:	The Astrophysical Journal
Materias:	Accretion Active galactic nuclei Gravitational instability Magnetohydrodynamics Magnetohydrodynamical simulations Quasars
Acceso en línea:	https://doi.org/10.3847/1538-4357/ae42bd
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