Fig. 12.
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Space motion of WISE1810 (red square) compared with the galactic velocities of L subdwarfs (blue squares) and M subdwarfs from the sample of Savcheva et al. (2014) with ζ ≤ 0.825 (grey dots). The 2σ dispersion of the disc, thick disc, and halo populations are drawn as the dash-dotted, dashed, and solid circles, respectively (Fuchs et al. 2009; Savcheva et al. 2014).
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