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Fig. 7
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3D velocity distributions of the particles in the GCs for ɡ1 and ɡ1+ɡ2 simulations at T = −5 Gyr (i.e. after approximately one two-body relation time) after inserting the ɡ2 component. The distributions are similar in all cases as the ɡ2 component represents a small fraction of the stars.
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