© 2001 The Hydra Consortium
Science Programme
First objects Chemistry, masses, formation redshifts
Supernovae SNe in small halos; OB associations
Star formation Looking at methods to both infer the number of stars being formed and feed the energy of star formation back into the simulation.
Galaxy Formation In both large-scale cosmological simulations and in models of clusters of galaxies.
X-ray emission Large adiabatic simulations of cluster formation and evolution, in association with the Virgo Consortium
Interstellar Medium Studies of the formation and evolution of the ISM