Fig. 3

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Aspect ratio for all disks with at least one measured surface height. The black dashed line is the fit to several Τ Tauri stars done by Avenhaus et al. (2018), while the red dash-dotted line is the fit to the SPHERE J-band data of HD 97048 from Ginski et al. (2016). Data points in gray and black have intrinsically very large uncertainties (not displayed, but shown in Table 3).
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