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...
Saved in:
| Main Authors: | D. Pugliese, Z. Stuchlík |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2024-01-01
|
| Series: | The Astrophysical Journal Supplement Series |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4365/ad8645 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Image of the Kerr–Newman Black Hole Surrounded by a Thin Accretion Disk
by: Sen Guo, et al.
Published: (2024-01-01) -
Near-horizon Polarization as a Diagnostic of Black Hole Spacetime
by: Yehui Hou, et al.
Published: (2025-01-01) -
Assessing the Role of Intrinsic Variability in Black Hole Parameter Inference Using Multiepoch EHT Data
by: Dominic O. Chang, et al.
Published: (2025-01-01) -
Multimessenger Probes of Supermassive Black Hole Spin Evolution
by: Angelo Ricarte, et al.
Published: (2025-01-01) -
Tidal Forces Around Black-Bounce-Reissner–Nordström Black Hole
by: Rashmi Uniyal
Published: (2025-07-01)