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

© 2001 The Hydra Consortium
last updated September 7, 2001