Fig. 11
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Normalised component width as a function of disc inclination. The dashed grey lines indicate the projected velocity of a purely Keplerian disc at the indicated radius. Plus markers and error bars have the same meanings as in Fig. 8. For the Pascucci et al. (2020) sample, stellar masses from Banzatti et al. (2019) and Fang et al. (2018) are used to normalise the [NeII] 12.81 μm line widths. Objects without available mass estimates are omitted.
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