Fig. A.6.
NGC 7193. Top left: Gaia DR2 proper motions for the members proposed by Angelo et al. (2019b) (blue dots) and Angelo et al. (2017) (cyan triangles). The error bars are smaller than the markers. The total proper-motion dispersion is indicated for both samples. Top right: parallax vs. G mag for the same stars. Middle row: same as top row, with a different scale. Bottom left: Gaia DR2 CMD for the same stars. Bottom right: radial velocity vs. G magnitude for the Angelo et al. (2017) stars.
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