Fig. 8.

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Column density Nion (top panel) and turbulent velocity, σv, (bottom panel) plotted versus the flow velocity, v, of the intrinsic UV absorption lines detected in the SUBWAYS HST sample. The data points correspond to the best-fit parameters of Table A.2. The σv is calculated from the FWHM of the absorption line according to . The Spearman’s rank correlation coefficient, rs, and the null hypothesis probability, pnull, are given in the inset. There is a statistically significant correlation between Nion and v, even including the four outlier data points on the far left, which belong to only one object (PG 1307+085). All data points with a positive value for v (i.e., inflow) belong to only one component of one object (Comp. 1 of PG 0804+761). All other targets show only outflows.
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