Fig. 1.
Distribution of the morphological types, absolute SDSS r-band magnitudes, circular velocities, disc inclinations, and bar radii of the initial sample of 31 CALIFA galaxies analysed with the TW method by Aguerri et al. (2015) and Cuomo et al. (2019a) (black solid line) and of the subsample of 12 galaxies hosting an ultrafast bar discussed in this paper (red dotted line).
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