Principal Investigator: Jenny G. Sorce(1), Klaus Dolag(2), (1) Leibniz-Institut für Astrophysik Potsdam/AIP (Germany) and Centre de Recherche Astrophysique de Lyon (France), (2) Universitäts-Sternwarte, Ludwig-Maximilians-Universität München (Germany)
HPC Platform used: SuperMUC of LRZ
Local Project ID: pr74do
The neighbourhood in the immediate vicinity of the Milky Way is known as the “Local Group”. It is a binary system composed of two averaged sized galaxies (the Milky Way and Andromeda) dominating a volume that is roughly ~7 Mpc in diameter. At a distance of around 15Mpc, the Virgo cluster comes into view as the main defining feature of our neighbourhood on these scales. Beyond Virgo, a number of well known and well observed clusters like Centaurus, Fornax, Hydra, Norma, Perseus and Coma dominate the night sky. This is our cosmic neighbourhood. The goal of this project is, for the first time, to perform targeted, state of the art hydro-dynamical simulations covering this special region of the universe and to compare the results with various...