Fig. 6
SEDs of several Fermi-LAT SNRs interacting with molecular clouds (blue tone colors) and being dynamically young (orange tone colors). The black stars correspond to the SED of G150.3+4.5 shown in Fig. 4 (right) using the disk model. References: RX J1713.7−3946 (H.E.S.S. Collaboration 2018a), RCW 86 (Ajello et al. 2016), Vela Junior (H.E.S.S. Collaboration 2018b), IC 443, and W44 (Ackermann et al. 2013).
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