Fig. 6
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Maximum morphological correlation between the 10° × 10° LOS velocity channels and the dust density in the range 69 < d < 1250 pc, as quantified by the direction-sensitive projected Rayleigh statistic (Vd; Eq. (2)). The cyan curves represent the vLOS expected for d = 69 and 1250 pc according to the Reid et al. (2019) Galactic rotation model, shown by dotted and dashed lines, respectively.
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