Practical formulae for the evaluation of the fluxes due to Compton scattering within discrete sources are derived. These formulae are used to predict the fluxes from M87, the Crab Nebula, M82, Cen A, NGC 1275, and Cas A. The predicted fluxes for certain models of M87, the Crab Nebula, and M82 are found to be above the sensitivities of gamma-ray-detection experiments now in preparation
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Rieke et al. (1969) studied this question.
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