Fig. 12
Fraction of galaxies with different values of the Pseudo-Ring attribute as a function of EFIGI morphological type for the 3105 galaxies with Inclination-Elongation ≤ 2. For clarity, no errorbars are plotted, as these are large due to the small number of objects (see Table 7). The outer pseudo-ring pattern is essentially present in S0+, S0a, Sa, Sab and Sb galaxies.
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