Fig. B.1.
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Orbits. Ensemble of 10 000 orbits for each studied star cluster by considering the errors on the observables, projected on the equatorial (top panels) and meridional (bottom panels) Galactic planes in the inertial reference frame, with a bar pattern speed of 31, 41, and 51 km s−1 and integrated over the past 2.0 Gyr. The red and orange colours correspond to more probable regions of the space, which are crossed most frequently by the simulated orbits. The black line shows the orbit of the star cluster from the observables without error bars. (a) ESO 92-18. (b) Ferrero 54. (c) Gaia 2. (d) Kronberger 99. (e) Kronberger 119. (f) Kronberger 143. (g) Patchick 122. (h) Patchick 125. (i) Patchick 126. (j) ESO 98-3. (k) VVV-CL60.
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