Image Details
Caption: Figure 2.
Comparison between the flux of high-energy ﹩{{\rm{e}}}^{-}﹩ CRs measured with AMS02 (Aguilar et al. 2014b) and the flux expected from Fermi acceleration in the source of ﹩{{\rm{e}}}^{-}﹩'s plus secondary production in/near source and in the ISM.
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