The effect of non-gravitational gas heating in groups and clusters of galaxies Journal Articles uri icon

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abstract

  • We present a set of gas-dynamical simulations of galaxy groups and clusters aimed at exploring the effect of non-gravitational heating. We use GASOLINE, a parallel Tree+SPH code, to simulate the formation of four cosmic halos with temperature 0.5

authors

  • Borgani, S
  • Governato, F
  • Wadsley, James
  • Menci, N
  • Tozzi, P
  • Quinn, T
  • Stadel, J
  • Lake, G

publication date

  • October 21, 2002