Abstract:X-ray emission of a pulsar wind nebula (PWN) is a group of particles with the highest energy among the non-thermal electron-positrons present in the nebula. The standard emission model of PWNe predicts that such high energy particles lose their energy immediately by radiative cooling and that the emission region of X-rays is smaller than those of lower frequencies. However, as 3C 58 and G21.5-0.9, some PWNe have been discovered in which the emission region of X-rays and radio extend to the almost same extent, … Show more
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