Fig. 8.
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Maximum momentum of accelerated particles at a young SNR shock expanding in the dense wind of the progenitor star, as a function of density and shock velocity. The green circles, crosses, and triangles show the typical values reached 1 day, 1 month, and 1 year after the SN explosion, respectively. The size of the symbols increases with Ṁ from 10−5 to 1 M⊙/yr.
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