Fig. 3.
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Nonthermal 1.4 GHz radio synchrotron emission maps (in erg s1 cm2 sr1 Hz1) for the pulsar wind nebulae and their host SNR, without (a,b) and with (c,d) CSM. The maps are displayed with a viewing angle of θincl = 0° (a,c) and θincl = 45° (b,d). The dark color marks the regions of strong emission intensity, while the pale color marks the regions of fainter radio emission intensity, respectively.
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