Fig. 3.
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Spectral energy distribution (SED) of the source detected by Fermi-LAT in correspondence of NGC 6611/M16. The error bars refer to the statistical 1σ uncertainties. The solid and dashed green lines represent the emission model in the case of Kraichnan turbulence, and the lines differ in the assumed wind luminosity, Lw, as indicated in the figure legend.
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