Fig. 12.
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Evolution of unbarred disc galaxies divided into two subsamples: unbarred galaxies at z = 1 that become barred galaxies at z = 0 (left column), and those that were not able to develop a stable bar structure at any point up to z = 0 (right column). Solid lines represent the median values and the shaded area corresponds to the 20th and 80th percentiles of the distribution.
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