Relation between the deconvolved HWHM normalised by the stellar mass and sin (i_disk) for the NLVC. Black lines indicate line widths as a function of inclination at disk radii of 0.2, 0.5, 2 and 5 au, in the assumption of Keplerian motion. In the upper panel, blue and cyan symbols distinguish sources where the V_p of the line is consistent with the origin in the disk or consistent with a wind, respectively. In the bottom panel, the distribution with respect to the disk type is shown, with colours code as in Fig. 4.