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Kinematic Map of the Galactic Bulge Using HST Proper Motions
Constraining the Galactic bulge's non-axisymmetric dynamics requires proper motions in deep fields across many sightlines, yet crowding and extinction limit such measurements. Using multi-epoch observations of 27 fields in the southern Galactic bulge (-6$^\circ$ < l < 4$^\circ$, -5$^\circ$ < b < -1$
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