Fig. 2.
Praesepe cluster and its tidal tails shown in the YP, Xp-plane (left) and the YP, Zp-plane (right). Stars selected in Gaia DR2 are shown as dots colour coded by their pcont-values (pcont < 0.015 in grey, pcont ≈ 0.1 in orange and pcont ≈ 0.5 in light green). The location of the simulated tidal tails from the model by Kharchenko et al. (2009) is indicated as beige-coloured structures.
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