Speaker
Jong-heun Kim
Description
The black hole accretion disks contain highly ionized Fe, including C$_{IV}$, N$_V$, and O$_{VI}$ at a temperature of about $10^8$K. The relatively hot accretion disk ($10^8$K) and the relatively cool surrounding medium ($10^6$K) are mixed and the iron is ionized and recombined to release the X-ray. This paper investigate the physical properties of turbulent mixing layers and the production of highly ionized irons, by using hydrodynamic simulations with radiative cooling and non-equilibrium ionization (NEI) calculations.
Primary author
Co-authors
Mr
Kwanghyun Sung
Dr
Kyujin Kawk
