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

public/chevalierfranssson-plan.txt · Last modified: 2015/10/21 10:14 by Stephen Smartt

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