Fig. 10.
On-sky positions and proper motions of the candidates from region C (red and green stars), along with the members ϵ Cha (black circles Murphy et al. 2013) and Gaia DR2-selected candidate members of LCC (coloured dots Goldman et al. 2018). The LCC sources are coloured according to the declination (top plots) and Gaia DR2 distance (bottom). The distances of ϵ Cha objects in this plot are in the range ∼93–110 pc, similar to our candidates (∼94–113 pc).
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