Phone: 54 351 433 1066 – Fax: Int. 101 – E-mail: iate@oac.unc.edu.ar – Laprida 854, Córdoba, Argentina
Expositor: Dra. Cinthia Ragone-Figueroa (IATE)
Date: 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
The 13.8 billion years of the Universe is enough time to form giant objects, being the galaxies one of the most interesting. Galaxies are truly island universes where […]
Read More
El Universo está plagado de estrellas y la mayoría de ellas forman sistemas estelares y asociaciones. Entre los muchos sistemas estelares que pueden observarse, los cúmulos estelares (CE) se encuentran […]
Read More
The large-scale structure of the Universe is the field of cosmology that studies the distribution of the matter in the Universe on the largest scales […]
Read More
The plasma is the most common state of the baryonic matter in the Universe (99%). Most of a star, the interplanetary and interstellar medium, and the ionosphere, are plasmas […]
Read More
Los estudios desarrollados por los integrantes del Grupo de Sistemas Planetarios buscan descifrar el origen y la evolución dinámica de planetas y cuerpos menores que orbitan el Sol u otras estrellas. […]
Read More
English 
Español de Argentina