Figure 2 from THE ORIGIN OF THE COSMIC GAMMA-RAY BACKGROUND IN THE MeV RANGE

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THE ORIGIN OF THE COSMIC GAMMA-RAY BACKGROUND IN THE MeV RANGE

Authors: Pilar Ruiz-Lapuente, Lih-Sin The, Dieter H. Hartmann, Marco Ajello, Ramon Canal, Friedrich K. Röpke, Sebastian T. Ohlmann, and Wolfgang Hillebrandt

2016 The Astrophysical Journal 820 142.

Provider: AAS Journals

Caption: Figure 2.

Total X-ray continuum and gamma-ray line fluxes per ⁵⁶Ni nuclei, integrated over the first 600 days comparing the calculations for the fully mixed W7 model (W7fm) used in W99b (blue line), for the (spherically averaged) delayed-detonation 3D model N100 of Röpke et al. (2012; green line), and for the (also averaged) 3D model of the violent merging of two WDs of Pakmor et al. (2012; red line).

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