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...

Descrición completa

Detalles Bibliográficos

Principais autores:	Hannalore J. Gerling-Dunsmore, Mitchell C. Begelman, Jacob B. Simon, Philip J. Armitage
Formato:	Artigo
Idioma:	Inglês
Publicado:	IOP Publishing 2026-01-01
Series:	The Astrophysical Journal
Assuntos:	Accretion Active galactic nuclei Gravitational instability Magnetohydrodynamics Magnetohydrodynamical simulations Quasars
Acceso en liña:	https://doi.org/10.3847/1538-4357/ae42bd
Tags:	Engadir etiqueta Sen Etiquetas, Sexa o primeiro en etiquetar este rexistro!