Change of ΔL of stars over time along the tangential distance to the cluster centre split up into the subsystems. Left panels: Stars from the BFSR. Right panels: Stars of the COSR. Dashed red lines show the impact of the stars in the cluster. Thick blue lines represent the stars in the tidal tails and dotted green lines indicate the stars between 1r_J radius and 2r_J. Dot-dashed black lines show the contribution to the angular momentum of the stars that were lost in the violent relaxation phase and thick amber lines represent the total of all contributions. The direct measurement was omitted for clarity, as it consistently coincided with the total. Note that the Y_cyl,loc-axis for the stars in the trailing arm (negative values) is flipped. The unit, δL_out, corresponds to kpc · km s⁻¹ and indicates the z-component of the star’s angular momentum relative to the cluster centre at escape.