The effect of Compton drag on the dynamics of dissipative Poynting-dominated flows: Implications for the unification of radio loud AGN

Keyphrases

• Active Galactic nuclei 100%
• Asymmetric Magnetic Field 50%
• Blazars 50%
• Collimating 50%
• Compton Scattering 50%
• Cooling Time 50%
• Current Sheet 50%
• Density Profile 50%
• Dissipated Energy 50%
• Dissipation Time 50%
• Field Dissipation 50%
• Flat Density 50%
• Gamma Rays 100%
• Initial Magnetization 50%
• Kink Instability 50%
• Local Dissipation 50%
• Lorentz Factor 100%
• Magnetic Energy 50%
• Magnetic Field 50%
• Magnetohydrodynamic Simulation 50%
• Polar Regions 50%
• Poynting 100%
• Poynting Flux 50%
• Radiative Efficiency 50%
• Radiative Loss 50%
• Radio Sources 50%
• Radio-loudness 100%
• Reconnecting 50%
• Relativistic Electrons 50%
• Riley 100%
• Stable Configuration 50%
• Synchrotron 100%

Physics

• Active Galactic Nuclei 100%
• Blazars 50%
• Compton Scattering 50%
• Current Sheet 50%
• Gamma Radiation 100%
• Magnetic Field 100%
• Magnetohydrodynamic Simulation 50%
• Radio Sources 50%
• Synchrotron 100%