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Leaked GeV CRs from a Broken Shell: Explaining 9 Years of Fermi-LAT Data of SNR W28

  • Authors: Yudong Cui, Paul K. H. Yeung, P. H. Thomas Tam, and Gerd Pühlhofer

2018 The Astrophysical Journal 860 69.

  • Provider: AAS Journals

Caption: Figure 7.

SNR evolution profiles. The same SNR age/velocity profile adopted in both the damping and non-damping models is shown as the green and red line. Because of the different acceleration efficiencies and neutral densities adopted in the two models, two different evolution profiles of the escape energy (blue solid and dashed lines) are presented.

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