Expositor: Dra. Cinthia Ragone-Figueroa (IATE)
Fecha: Viernes 1 de Junio de 2018, 11 hs, Auditorio IATE.
Resumen: We analyze the stellar growth of Brightest Cluster Galaxies (BCGs) produced by cosmological zoom-in hydrodynamical simulations of the formation of massive galaxy clusters. The evolution of the stellar mass content is studied considering different apertures, and tracking backwards either the main progenitor of the z = 0 BCG or that of the cluster hosting the BCG at z = 0