Acceleration of cosmic rays at the post-adiabatic shocks of supernova remnants

Open Access

Fig. 3

Distances x_A and x_B from the shock for the two models. The flow speed u₂ < 0 between the two solid lines. The vertical dotted lines mark the times 1.49t_tr and t_sf. The flow speed u₂ > 0 in the whole domain before 1.49t_tr.

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