Dynamical Properties of Magnetized Low-angular-momentum Accretion Flows around a Kerr Black Hole
IK Dihingia, Y Mizuno - The Astrophysical Journal, 2024 - iopscience.iop.org
An essential factor for determining the characteristics of an accretion flow is its angular
momentum. According to the angular momentum of the flow, semi-analytical analysis …
momentum. According to the angular momentum of the flow, semi-analytical analysis …
Time delays between radio and X-ray and between narrow radio bands of Sgr A* flares in the shock oscillation model
We examine the time delay between radio and X-ray and between narrow radio frequency
flares in Sagittarius A*(Sgr A*), from analyses of the synchrotron, bremsstrahlung, and …
flares in Sagittarius A*(Sgr A*), from analyses of the synchrotron, bremsstrahlung, and …
Evolution of MHD torus and mass outflow around spinning AGNs
We perform axisymmetric, 2D magnetohydrodynamic simulations to investigate accretion
flows around spinning active galactic nuclei. To mimic the space–time geometry of spinning …
flows around spinning active galactic nuclei. To mimic the space–time geometry of spinning …
Radiation RMHD accretion flows around spinning AGNs: a comparative study of MAD and SANE state
In our study, we examine a 2D radiation, relativistic, magnetohydrodynamics (Rad-RMHD)
accretion flows around a spinning supermassive black hole. We begin by setting an initial …
accretion flows around a spinning supermassive black hole. We begin by setting an initial …