The rise and fall of bars in disc galaxies from z = 1 to z = 0 - The role of environment

Open Access

Fig. 2.

D/T distribution of disc galaxies at z = 1 (top panel) and their descendants at z = 0 (bottom panel). We note that there was a morphological transformation overall in the population of the descendants of parent disc galaxies, especially for the thin disc component.

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