Fig. 5

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X-ray and radio intensity profiles of PWN PSR J2030+4415 as a function of the distance from PSR J2030+4415. The cutting line that defines the profile scans crosses the pulsar position and follows the proper motion direction of the pulsar (PA= 7.2°). The grey line corresponds to 0.5–7 keV X-ray data, whereas the blue line corresponds to the radio data at 736 MHz and the green line to the 1274 MHz data, with the common synthesized beam of 6″ × 6″. The vertical red dashed line marks the pulsar position. We note that the small X-ray peaks far from the pulsar also represent significant emission.
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