Fig. 5

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Limits on the width of the 26Al line emission from ROIs around the Galactic centre with an extent in latitude of ±6° and longitude extents ranging from 6° to 128°. The error bars of decreasing thickness show the Bayesian highest posterior density credible regions corresponding to 68.3%, 95.4%, and 99.7%, corresponding to 1σ, 2σ, and 3σ.

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