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Photon Shells, Black Hole Shadows, and Accretion Toroids

We analyze the properties of the Kerr black hole (BH) photon shell, focusing on the influence of aggregates of corotating and counterrotating toroids (ringed accretion disks, hereafter RAD), orbiting in the BH photon shell (photon shell “obscuration”). The particular case of a corotating accretion d...

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Detalles Bibliográficos
Principais autores: D. Pugliese, Z. Stuchlík
Formato: Artigo
Idioma:Inglês
Publicado: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Supplement Series
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Acceso en liña:https://doi.org/10.3847/1538-4365/ad8645
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