Fig. 7.

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Gamma-ray spectra of the PWN, SNR, and ISM components at 10 kyr in a high-turbulence case, as a function of the maximum particle momentum allowed in the remnant. The PWN emission is the same in all three runs since it is not affected by this parameter. The gray dotted line corresponds to an order-of-magnitude estimate of the pion-decay emission from cosmic rays in the remnant (see text for details).
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