Spatial distribution and VPD for the 32 Ori MG members. Top: Spatial distribution of the known members from Bell et al. (2017), after removing some outliers. The two populations based on parallaxes are shown. Bottom: VPD of the 32 Ori MG, sub-sample red squares are population 1 (ϖ < 9.52 mas) and blue circles population 2 (ϖ > 9.52 mas). Black dashed ellipses are the Pleiades members taken from Gaia Collaboration 2018b and the light grey plus symbols are the Taurus-Auriga members taken from Ducourant et al. (2005). The proper motion data have been taken from the Gaia DR2 catalogue, with the exception of the Taurus sample that comes from Ducourant et al. (2005).