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On the Radio-emitting Particles of the Crab Nebula: Stochastic Acceleration Model

  • Authors: Shuta J. Tanaka, and Katsuaki Asano

2017 The Astrophysical Journal 841 78.

  • Provider: AAS Journals

Caption: Figure 4.

Calculation results of Model 2: the current photon spectrum (top left), the evolution of the particle spectra (top right), the timescales (bottom left), and the evolution of the fractional energy (bottom right). See the caption in Figures 1 and 3 for details. Model 2 adopts Qext = Qimp and finite values of τturb and γcut in Equation (5). The used parameters are summarized in Table 1.

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