Figure 4.
The distributions of vϕ for red-clump giants (black data points) and fits to them – in each panel the dashed curve shows the kinematic model specified by equations (7) and (8), while the full curve shows the model convolved with the mean errors in vϕ. The red points show the predictions of the B12 dynamical model. The mean coordinates of the stars in each bin are given at top left, followed by the rms velocity error (eV) and the sample mean of vϕ (vbar). In this and all subsequent histograms, the horizontal bars span the width of the bins and the vertical bars indicate Poisson errors.

The distributions of vϕ for red-clump giants (black data points) and fits to them – in each panel the dashed curve shows the kinematic model specified by equations (7) and (8), while the full curve shows the model convolved with the mean errors in vϕ. The red points show the predictions of the B12 dynamical model. The mean coordinates of the stars in each bin are given at top left, followed by the rms velocity error (eV) and the sample mean of vϕ (vbar). In this and all subsequent histograms, the horizontal bars span the width of the bins and the vertical bars indicate Poisson errors.

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