Fig. 12.

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A suggested model for the SED including a secondary electron contribution located at the shock position. The low and high state spectra as measured with Fermi-LAT are shown for comparison (Yeung & Horns 2020). The secondary electrons’ spectrum during average (high) state is a power-law with dn/dγ ∝ γ−2.3 between γ1 = 3 × 109 and γ2 = 7(18)×109. The magnetic field in the region is chosen to be 85 μG. The total energy content of the electrons is 2(3)×1042 ergs. The dotted lines indicate the effect of absorption on the Galactic foreground emission (see also Appendix B).
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