On the Viscous Ringed Disk Evolution in the Kerr Black Hole Spacetime
Supermassive black holes <b>(SMBHs)</b> are observed in active galactic nuclei interacting with their environments, where chaotical, discontinuous accretion episodes may leave matter remnants orbiting the central attractor in the form of sequences of orbiting toroidal structures, with strongly diffe...
Gardado en:
| Principais autores: | , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
MDPI AG
2024-11-01
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| Series: | Universe |
| Assuntos: | |
| Acceso en liña: | https://www.mdpi.com/2218-1997/10/12/435 |
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