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Fig. 7


BRC and FRC are compared with respect to the kinematical model for a strong boxy-peanut bulge (Debattista et al. 2005). From the model, two samples were selected from the two overdensities formed by the near (red) and far (blue) arms of the boxy-peanut stellar distribution, in the line of sight for (l,b) = (0, −6). Color lines over U, V, and W histograms correspond to the median value for each distribution.

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