Fig. 9.
Modelling the H I rotation curve of the Fourcade-Figueroa galaxy. Upper panels: ISO and the NFW halo based mass model for the minimum disk + gas. Lower panels: ISO and the NFW halo based mass model for the FF galaxy for the minimum disk. The orange line indicates the rotation curve due to the stellar disk, the blue line that due to the gas disk, the green line that due to the DM halo, and red shows the best-fitting model rotation curve.
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