Fig. 7.
Red and blue solid lines: observed 2 to 50 pc radial fluxes in Ks and H band; red and blue dashed lines: Ks-band and H-band profiles resulting from our radiative transfer model, when the power law for the stellar and dust radial density have exponents of −4.20 and −1.05, respectively. The result is a quasi-power law for both brightness profiles.
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