Fig. 15.
Projected velocity distributions of member stars (Sect. 4). The hatched bins show stars that highly deviate from the samples means after applying a sigma-clipping routine. Open histograms were employed to calculate σvp and σv. Poisson uncertainties are also shown. Histograms are shown for NGC 2180, Lynga 8, Bica 5, NGC 7036, Alessi 3, and ESO 426-SC26.
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