Fig. 8

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Two-panel visualisation of the disk vertical height (h) and aspect ratio (h/r) as a function of separation (r) for extended disks only (with a total extent of >150 au). R2 is shown the in bottom right corner of each plot. Top: power-law fit to h vs. r shows an increasing vertical structure consistent with flaring. Bottom: h/r vs. r with power-law fits overlaid for this work (black), and comparison to Avenhaus et al. (2018) and Ginski et al. (2016) shown in grey and light blue respectively.
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