Synchrotron self-absorption alters radiation-mediated shock profiles for magnetizations above 10^{-8}, subshocks appear above 0.1, and hadronic processes add a high-energy photon tail with negligible effect on overall shock dynamics.
Fermi, On the Origin of the Cosmic Radiation, Phys- ical Review75, 1169 (1949)
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Magnetized Shocks Mediated by Radiation from Leptonic and Hadronic Processes
Synchrotron self-absorption alters radiation-mediated shock profiles for magnetizations above 10^{-8}, subshocks appear above 0.1, and hadronic processes add a high-energy photon tail with negligible effect on overall shock dynamics.