The aluminium-26 distribution in a cosmological simulation of a Milky Way-type Galaxy

Open Access

Fig. 4

Same as Figure 2, but color-coded as function of the number of emitted 1.8 MeV γ-rays per second by each gas particle, as seen by the observer. The outer (inner) black contour representing the 100 km/s (200 km/s) threshold (as in Figure 2) are retained here as a visual guide.

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