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The Relativistic Outflow Driven by the Large-scale Magnetic Field from an Accretion Disk

Outflows/jets are ubiquitous in a wide range of astrophysical objects, yet the mechanisms responsible for their generation remain elusive. One hypothesis is that they are magnetically driven. Based on general relativistic MHD equations, we establish a formulation to describe the outflows driven by l...

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Detalhes bibliográficos
Principais autores: Wei Xie, Wei-Hua Lei
Formato: Artigo
Idioma:Inglês
Publicado em: IOP Publishing 2025-01-01
coleção:The Astrophysical Journal
Assuntos:
Acesso em linha:https://doi.org/10.3847/1538-4357/adc100
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