The multidimensional structure of radiative shocks: Suppressed thermal X-rays and relativistic ion acceleration

Keyphrases

• 1D Analysis 20%
• Acceleration Efficiency 20%
• Angle Distribution 20%
• Astrophysical Transients 20%
• Average Acceleration 20%
• Circumstellar Material 20%
• Classical Novae 20%
• Cold Filament 20%
• Dense Layer 20%
• Diffusive Shock Acceleration 20%
• Field Geometry 20%
• Gamma Rays 20%
• Heat Conduction 20%
• High Mach number 20%
• Hydrodynamic Simulation 20%
• Inclination Angle 20%
• Ion Acceleration 100%
• Ion Energy Spectrum 20%
• Local Region 20%
• Luminosity 20%
• Magnetic Field 20%
• Multidimensional Structure 100%
• Novae 20%
• Numerical Techniques 20%
• Optically Thin 20%
• Parallel Magnetic Field 20%
• Particle-in-cell Simulation 20%
• Quasi-parallel 20%
• Radiative Shocks 100%
• Relativistic Heavy Ions 100%
• Shell Instability 20%
• Shock 100%
• Shock Front 20%
• Supernovae 20%
• Thermal Acceleration 20%
• Thermal Energy 20%
• Thermal Radiation 20%
• Thin Shell 20%
• Weak Shock 20%
• X-ray 100%

Physics

• Classical Novae 50%
• Conductive Heat Transfer 50%
• Energy Spectra 50%
• Gamma Radiation 50%
• Hydrodynamical Simulations 50%
• Mach Number 50%
• Magnetic Field 100%
• Novae 50%
• Shock Front 50%
• Supernovae 50%
• Thermal Radiation 50%
• Transients 100%