Jet Formation in 3D GRMHD Simulations of Bondi–Hoyle–Lyttleton Accretion

A black hole (BH) traveling through a uniform, gaseous medium is described by Bondi–Hoyle–Lyttleton (BHL) accretion. If the medium is magnetized, then the black hole can produce relativistic outflows. We performed the first 3D, general-relativistic magnetohydrodynamic simulations of BHL accretion on...

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Autors principals:	Nicholas Kaaz, Ariadna Murguia-Berthier, Koushik Chatterjee, Matthew T. P. Liska, Alexander Tchekhovskoy
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2023-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	High energy astrophysics Relativistic jets Astrophysical black holes Bondi accretion Stellar winds
Accés en línia:	https://doi.org/10.3847/1538-4357/acc7a1
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