2 papers
astro-ph1997
Cooling Limits on Galaxy Formation; Gas dynamical simulations incorporating a background UV field and metal enrichment
John Hultman, Daniel Kaellander
We present hydrodynamical simulations of the formation of galaxies in the mass range 10^9 - 10^13 solar masses, with the focus on the efficiency of gas cooling. The effect of a bac…
astro-ph1997
An SPH code for galaxy formation problems; Presentation of the code
John Hultman, Daniel Kaellander
We present and test a code for two-fluid simulations of galaxy formation, one of the fluids being collision-less. The hydrodynamical evolution is solved through the SPH method whil…