Evolution of galaxies in groups in the Coma Supercluster

摘要: We take a close look at the galaxies in Coma Supercluster and assess role of environment (in form cluster, group supercluster filament) their evolution, particular examining groups. characterise groups according to intrinsic properties such as richness halo mass, well position proximity two rich clusters, Abell 1656 (Coma) 1367. devise new way characterising local using kernel density estimator. find that apart from dominant effects galaxy effect on is complex combination overdensities various scales, which characterised terms membership groups, also filaments infall regions clusters. Whether gas can be turned into stars depends upon level pre-processing, plays how star formation enhanced given environment. Our results are consistent with accreted cold mode filaments, being made available enhance formation. Finally, we show Abell~1367 end process assembly present, leading heightened activity, contrast Coma-end filament system.