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Investigating the Pulsar Wind Nebula 3C 58 Using Emission Models

An, Hongjun; Park, Jaegeun; Kim, Seungjong

We present IR flux density measurements, models of the broadband SED, and results of SED modeling for the Pulsar Wind Nebula (PWN) 3C 58. We find that the Herschel flux density seems to be slightly lower than suggested by interpolation of previous measurements in nearby wavebands, implying that there may be multiple electron populations in 3C 58. …