Fig. B.3

Simulated γ-ray spectra from hadronic collisions of CRs inside MC-J1729 (solid lines) and MC-core (dashed lines). The spectra are obtained through multiplication of the simulated CR density at 30 pc (100 pc) with the total mass of MC-J1729 (MC-core) for the 20 M⊙ SN IIL/b (blue) and the 25 M⊙ SN Ib/c (cyan) scenarios. Observational data from Abramowski et al. (2011) for HESS J1729-345 are shown as black circles.
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