Imprints of Different Types of Low-angular-momentum Accretion Flow Solutions in General Relativistic Hydrodynamic Simulations
Depending on the astrophysical source and its environment, the accretion flows can exhibit a variety of behaviors and characteristics in accordance with the type of solutions. We study low-angular-momentum accretion flows onto black holes using 2D general relativistic hydrodynamic simulations to fin...
Saved in:
| Main Authors: | Indu K. Dihingia, Akhil Uniyal, Yosuke Mizuno |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/adf221 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Emergence of cHz Quasiperiodic Oscillations from a Low-angular-momentum Flow onto a Supermassive Black Hole
by: Indu K. Dihingia, et al.
Published: (2025-01-01) -
Low-angular-momentum Black Hole Accretion: First General Relativistic Magnetohydrodynamic Evidence of Standing Shocks
by: Jirong Mao, et al.
Published: (2025-01-01) -
NICER Spectral and Timing Analysis of 4U 1630-47 and Its Heartbeat State
by: Ningyue Fan, et al.
Published: (2025-01-01) -
Is the Spin of the Black Hole in GX 339–4 Negative?
by: Andrzej A. Zdziarski, et al.
Published: (2025-01-01) -
The Impact of Plasma Angular Momentum on Magnetically Arrested Flows and Relativistic Jets in Hot Accretion Flows around Black Holes
by: Ho-Sang Chan, et al.
Published: (2025-01-01)