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Fig. 6.

image

Left: G magnitude distribution of all the OBA stars selected in Sect. 2.1 (orange histogram) and of the sources selected in Sect. 3 (grey histogram), with astro-kinematic distances comparable with those estimated by Bailer-Jones et al. (2018). Right: absolute magnitude distribution of all the OBA stars selected in Sect. 2.1, computed using their parallax (orange histogram), and of the sources selected in Sect. 3, computed using their astro-kinematic distances (grey histogram).

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