Figure 3 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 3.

Total time-integrated X-ray continuum and gamma-ray line fluxes per ⁵⁶Ni nucleus, comparing the calculations for an average model of the sub-Chandrasekhar pure detonation models (Sim et al. 2010; Ruiter et al. 2013; red line) and for the W7fm model of W99b (blue line).

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