Fig. D.2.
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Three different fit results to the spectral energy distribution (SED) of the source detected by Fermi-LAT in correspondence of NGC 6611/M16. The solid and dashed curve differ in the assumed wind luminosity, Lw, as indicated in the figure legend. The three different panels refer to the three turbulence spectra assumed: Kolmogorov (red), Kraichnan (green), and Bohm (blue).
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