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Fig. 9

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Deprojected [O i]630nm HVC peak velocities as a function of Lacc for the GHOsT subsample driving jets (colored points) compared with a CTTs sample reported in Banzatti et al. (2019; black points). A fit to both data samples is shown as the dashed black line (Banzatti et al. 2019 sample) and as the continuous black line (GHOsT sample). The latter was computed by excluding the outliers (V409 Tau and FT Tau). The Pearson coefficient for the GHOsT distribution is labeled in the figure.

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