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- W2013526783 abstract "We present a radially symmetric leptonic model which allows to reproduce the spectral properties of the X-ray emission of several regions inside a young PWN. Using the optimized model parameter values obtained from the X-ray analysis, it is possible to calculate the IC emission of the lepton population and compare it with the data in the very high-energy range (E > 100GeV). This method has been applied to three young PWNe, namely MSH15−52, G0.9+0.1, and G21.5−0.9." @default.
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- W2013526783 date "2012-01-01" @default.
- W2013526783 modified "2023-10-10" @default.
- W2013526783 title "A model to reproduce the emission of young pulsar wind nebulae" @default.
- W2013526783 doi "https://doi.org/10.1063/1.4772266" @default.
- W2013526783 hasPublicationYear "2012" @default.
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