Autores
                Prof.
            
                        Joop Schaye
            
  Fecha y hora
                                    8 Oct 2015 - 10:30 Europe/London
                            Dirección
                                    Aula
Idioma de la charla
                                    Inglés
                            Número en la serie
                                    1
                            Descripción
                                    The realism of hydrodynamical simulations of the formation and evolution of galaxies has improved considerably in recent years. I will try to give some insight into the reasons behind this success, focusing in particular on the importance of subgrid models and the associated limitations. I will also present recent results from the cosmological EAGLE simulations as well as from higher-resolution simulations of individual galaxies.