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Winds and Disk Turbulence Exert Equal Torques on Thick Magnetically Arrested Disks

The conventional accretion disk lore is that magnetized turbulence is the principal angular momentum transport process that drives accretion. However, when dynamically important large-scale magnetic fields thread an accretion disk, they can produce mass and angular momentum outflows, known as winds...

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Principais autores: Vikram Manikantan, Nicholas Kaaz, Jonatan Jacquemin-Ide, Gibwa Musoke, Koushik Chatterjee, Matthew Liska, Alexander Tchekhovskoy
Formato: Artigo
Idioma:Inglês
Publicado em: IOP Publishing 2024-01-01
coleção:The Astrophysical Journal
Assuntos:
Black holes
High energy astrophysics
Accretion
Relativistic jets
Relativistic disks
Acesso em linha:https://doi.org/10.3847/1538-4357/ad323d
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