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We demonstrate that there is a clear statistical correlation between the (X, Y, Z, Vᵣ) phase-space distribution of the outer halo Galactic globular clusters (having 10 kpc = 10 kpc) clusters. The Sgr dSph was therefore not only an important contributor to the halo field star population, but it also had a significant role in the building-up of the globular cluster system of the Milky Way.
Bellazzini et al. (Wed,) studied this question.
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