Fig. 9
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Spatial distribution of a Gaia DR3 XP sample of 376 321 B star candidates (selected as 4.0 < xgbdist_logteff_mean < 4.5 & xgbdist_logg_mean < 6 &xgbdist_logteff_std < 0.1 & xgbdist_logg_std < 0.5) . Known over-densities corresponding to OB associations are annotated. The dotted ellipses correspond to (potential) star formation voids.
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