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Fig. 19.

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Theoretical rotation curve derived from Eq. (4), using parameters from Table 1. The contributions are from the nucleus (green), the bulge (blue), the stellar disk (orange), the gaseous disk (red), and the dark matter halo (purple). The black line is the total rotation curve. The blue triangles correspond to the measured ionized gas velocities, averaged over the NE and SW side, and corrected from asymmetric drift.

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