Fig. 10.

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Probability density in the equatorial Galactic plane (top) and side-on (bottom) of 100 000 simulated orbits of FSR 1776 time-integrated backward for 1 Gyr. Yellow–orange corresponds to more probable regions of the space more frequently crossed by the simulated orbits. The black line refers to the cluster orbit computed with the central observable. The white star gives the current position of FSR 1776.
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