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Spectral energy distribution modeling of broadband emission in the pulsar wind nebula 3C 58
DOI: 10.1002/asna.202023774 Bibcode: 2020AN....341..170K

An, Hongjun; Kim, Seungjong

We investigate the broadband emission properties of the pulsar wind nebula (PWN) 3C 58 using a spectral energy distribution (SED) model. We attempt to match simultaneously the broadband SED and spatial variations of X‑ray emission in the PWN. We further use the model to explain a possible far‑IR feature of which a hint was recently suggested in 3C…

2020 Astronomische Nachrichten
Herschel 4