Fig. 9
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Relative rms error for the model fits using the COM, CMM, and AMMI dust models. Errors are plotted against the FWHM (x-axis) and AV (y-axis) parameters. The data correspond to region C (cſ. Fig. 1). The diameter of the symbols is proportional to the squared error. Models with larger LOS extent and/or more extincted radiation fields tend to result in better fits.
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