Abstract
Important processes for continuum emission at γ-ray energies are bremsstrahlung, magneto-bremsstrahlung, and Compton scattering of blackbody radiation by energetic electrons and positrons [1–6].
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Lingenfelter, R.E., Rothschild, R.E. (2002). γ-Ray and Neutrino Astronomy. In: Cox, A.N. (eds) Allen’s Astrophysical Quantities. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-1186-0_10
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