We will present a preliminary 3D map of the nearest cluster to the Sun, the Hyades. We will combine the Gaia DR2 release for stellar members (Mass > 0.1 Msun) with ground-based infrared parallaxes obtained with the 2-m Liverpool telescope for eight L and T dwarf members (M = 0.05-0.08 Msun) of the Hyades. We will present a revised membership list and compare the spatial distribution of brown dwarfs with those of high-mass and low-mass stars.