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We analyze the dependence of galaxy evolution on cluster dynamical state andgalaxy luminosities for a sample of 146 galaxy clusters from the Yang SDSScatalog. Clusters were split according to their velocity distribution inGaussians (G) and Non-Gaussians (NG), and further divided by luminosity regime.We performed a classification in the Age-SSFR plane providing three classes:star-forming (SF), passive (PAS), and intermediate (GV -- green valley). Weshow that galaxies evolve in the same way in G and NG systems, but also suggestthat their formation histories leads to different mixtures of galactic typesand infall patterns. Separating the GV into star-forming and passivecomponents, we find more bright galaxies in the passive mode of NG than in Gsystems. We also find more intermediate faint galaxies in the star-formingcomponent of NG than in G systems. Our results suggest the GV as the stagewhere the transition from types Sab and Scd to S0 must be taking place, but theconversion between morphological types is independent of the dynamical stage ofthe clusters. Analyzing the velocity dispersion profiles, we find that objectsrecently infalling in clusters have a different composition between G and NGsystems. While all galaxy types infall onto G systems, Sab and Scd dominate theinfall onto NG systems. Finally, we find that faint Scd in the outskirts of NGsystems present higher asymmetries relative to the mean asymmetry of fieldgalaxies, suggesting environmental effects acting on these objects.

Classification and Evolution of Galaxies According to the Dynamical State of Host Clusters and Galaxy Luminosities