Axisymmetric Jeans modeling overestimates the Milky Way inner circular speed by ~4% due to bar-induced non-axisymmetric streaming.
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Axisymmetric Jeans modelling systematically overestimates the circular speed in the inner Milky Way
Axisymmetric Jeans modeling overestimates the Milky Way inner circular speed by ~4% due to bar-induced non-axisymmetric streaming.