Chap. 6 X-ray and radio emission from circumstellar interaction (Chevalier & Fransson)
1. Introduction 2. Initial conditions
2.1 Ejecta structure
2.2 Ambient medium
3. Shock interaction
3.1 Shock structure and evolution
3.2 Postshock conditions and radiative cooling
3.3 X-ray emission from hot gas
3.3.1 Optically thin emission
3.3.2 Absorption and scattering processes
3.4 Reprocessing of X-rays
4. Relativistic particles
4.1 Particle acceleration in shocks
4.2 Magnetic field amplification in shocks
4.3 Synchrotron emission
4.3.1 Optically thin emission
4.3.2 Absorption processes
4.4 Inverse Compton X-ray emission
5. Emission from supernovae 5.1 Type II
5.2 SN 1987A
5.3 Type Ib/c
5.4 Type Ia
6. Conclusions