Fig. 1.
Distribution of the morphological type (left panel), redshift (central panel), and absolute r band magnitude (right panel) of our sample of 29 bona fide SAB galaxies (black solid line), the sample of 16 SAB galaxies successfully analysed with the TW method (red dot-dashed line), and the 14 SAB galaxies hosting a non-ultrafast bar (green dashed line).
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