Fig. 10.
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Analogous to Fig. 9, except for a sample of 1.05 million red giants with [Fe/H] > −0.5 in the 2.8−3.2 kpc distance bin. Note that observed proper motions are much smaller due to about six times larger distances, while radial velocity variation with galactic longitude is much stronger due to the projection effects of the rotational velocity component.
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