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Fig. 14.
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Latitudinal velocity components, |vθ|, as a function of the galactocentric distance, r, of 4 M⊙ HVSs in QUMOND with γ = 1 (orange dots) and γ = 2 (red dots), and in Newtonian gravity with a spherical dark matter halo (qz = 1) (black dots).
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