Fig. 6
Ratio between VNCM = VROTCUR−Vexpected and Vexpected as a function of radius for the gSb, iSb and dSb models. The vertical dashed lines show 0.5, 1 and 2rbar estimated from the Fourier decomposition. Each rotation curve was derived from mock galaxies with projected bar orientation between 0 and 90 degrees. The projected bar PA are shown on top of each figure.
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