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Fig. 9

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Spectral evolution of the γ-ray emissivities per gas nucleon in the Eridu (green), Reticulum (red), and North Hydrus (cyan) clouds. The orange curve gives the average qLIS emissivity measured in the atomic gas at latitudes 10° ≤ |b| ≤ 70° (Casandjian 2015). The emissivities are shown for the HI optical-depth correction that best fits the γ-ray data (Ts = 100 K for Eridu, 140 K for qLIS, and optically thin for the others). The shaded bands include the statistical and systematic uncertainties.

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