Two-Temperature Magnetohydrodynamics Simulations of Propagation of Semi-Relativistic Jets
In astrophysical jets observed in active galactic nuclei and in microquasars, the energy exchange rate by Coulomb collision is insufficient for thermal equilibrium between ions and electrons. Therefore, it is necessary to consider the difference between the ion temperature and the electron temperatu...
Hlavní autoři: | Takumi Ohmura, Mami Machida, Kenji Nakamura, Yuki Kudoh, Yuta Asahina, Ryoji Matsumoto |
---|---|
Médium: | Článek |
Jazyk: | English |
Vydáno: |
MDPI AG
2019-01-01
|
Edice: | Galaxies |
Témata: | |
On-line přístup: | http://www.mdpi.com/2075-4434/7/1/14 |
Podobné jednotky
-
Particles in Relativistic Magnetohydrodynamic Jets. II. Bridging Jet Dynamics with Multi–wave band Nonthermal Emission Signatures
Autor: Ravi Pratap Dubey, a další
Vydáno: (2024-01-01) -
The Kelvin–Helmholtz Instability at the Boundary of Relativistic Magnetized Jets
Autor: Anthony Chow, a další
Vydáno: (2023-01-01) -
Particles in Relativistic MHD Jets. I. Role of Jet Dynamics in Particle Acceleration
Autor: Ravi Pratap Dubey, a další
Vydáno: (2023-01-01) -
Linear Stability Analysis of Relativistic Magnetized Jets: Methodology
Autor: Nektarios Vlahakis
Vydáno: (2023-08-01) -
How to Turn Jets into Cylinders near Supermassive Black Holes in 3D General Relativistic Magnetohydrodynamic Simulations
Autor: Valeriia Rohoza, a další
Vydáno: (2024-01-01)