Evolution of dust in the Orion Bar with Herschel - I. Radiative transfer modelling

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Fig. 12

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Solid line: SED extracted from the radiative transfer model using diffuse ISM properties (Table 2) at the 70 μm peak position (Fig. 9). Square: integrated fluxes in Herschel bands. Dotted line: modified blackbody fitted to the data.

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