Fig. 10
Hypothetical gaseous rotation curve of the Milky Way (solid line) after correcting for the initial velocity profile of Fig. 3. The cyan, pink, and gray shaded areas are the 1, 2, and 3σ confidence levels. Open circles are rotation velocities of masers from Reid et al. (2014). The dashed line is the power-law rotation curve model of the Galaxy from Bovy et al. (2012).
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