Fig. 2
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Gaia data of cluster members. (a) Top left: sky positions of cluster members of λ Ori from Cantat-Gaudin et al. (2020). Here, sources with a membership probability of 1.0 are plotted in red, 0.9 in green, 0.8 in blue, and 0.7 in grey. Sources with RVs from Tsantaki et al. (2022) are plotted as crosses. (b) Top right: Gaia EDR3 BP-RP versus Gmag colour-magnitude diagram. (c) Bottom left: Gaia EDR3 parallax versus RV. (d) Bottom right: Gaia EDR3 proper motions of the sources.
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