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Fig. 8


Models of HD 97048 with very small grains added to the disk. We note that a larger inner disk of 0.3–5 AU is chosen in this modeling grid to fit the observations. The higher the abundance of VSG, the larger the N-band size. The grey and light cyan boxes and the error bars indicate the ±1 error on the FWHM of the azimuthally averaged radial brightness profiles for the target and PSF, respectively. Observed data of HD 97048 is from Doucet et al. (2006).

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