Fig. 7
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Ellipses fitted to the radial sub-structures traced in scattered light (top) and resulting height of the scattering surface of the disk (bottom). We compare the scattering surface height with the average surface height profile of several T Tauri stars found by Avenhaus et al. (2018) and the extreme flaring case of the Herbig star HD 97048, discussed by Ginski et al. (2016).
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