作者: D.F. Torres , A. Cillis , J. Martín , E. de Oña Wilhelmi
DOI: 10.1016/J.JHEAP.2014.02.001
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摘要: Abstract The increasing sensitivity of instruments at X-ray and TeV energies has revealed a large number nebulae associated with bright pulsars. Despite this data set, the observed pulsar wind (PWNe) do not show uniform behavior main parameters driving features like luminosity, magnetization, others are still fully understood. To evaluate possible existence common evolutive trends to link characteristics nebula emission those powering pulsar, we selected sub-set 10 detections which likely ascribed young PWNe model spectral energy distribution time-dependent description nebulae's electron population. In 9 these cases, detailed model, using up-to-date multiwavelength information, is presented. best-fit discussed, together characteristics. We conclude that particle-dominated objects multiplicities, in general far from magnetic equipartition, relatively photon field enhancements required explain high level Comptonized photons observed. find significant correlations between efficiencies different frequencies magnetization. injection appear be particularly correlated properties either. normalized comparison SEDs (e.g., corresponding spin-down flux) same age significantly reduces distributions dispersion.