Evolution of High-energy Electron Distribution in Pulsar Wind Nebulae

In this paper, we analyze the spectral energy distributions (SEDs) of 17 powerful (with a spin-down luminosity greater than \(10^{35}\) erg s\(^{-1}\)) young (with an age less than 15000 yrs) pulsar wind nebulae (PWNe) using a simple time-independent one-zone emission model. Our aim is to investigat...

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Veröffentlicht in:	arXiv.org 2024-07
Hauptverfasser:	Yi-Ming, Liu, Hou-Dun Zeng, Yu-Liang, Xin, Si-Ming, Liu, Zhang, Yi
Format:	Artikel
Sprache:	eng
Schlagworte:	Age Correlation Electron distribution Electron energy Energy Evolution High energy electrons Luminosity Nebulae Pulsars Spectral energy distribution Stellar winds
Online-Zugang:	Volltext
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