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- W1640261098 abstract "We present results from a Smoothed Particle Hydrodynamic (SPH) simulation of galaxy formation that exceeds the minimum resolution requirement suggested by Steinmetz & Muller (1993) of 3*10^4 SPH particles per galaxy. Using the multiple mass technique an effective resolution of a little over one billion particles is attained within a 48 Mpc cube. We find that even with an SPH mass resolution of 1.5*10^6 solar masses and a plausible feedback algorithm, the cooling catastrophe continues to be a problem for Einstein-de Sitter CDM cosmologies. Increasing resolution also appears to exacerbate the core-halo angular momentum transport problem." @default.
- W1640261098 created "2016-06-24" @default.
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- W1640261098 date "2000-01-14" @default.
- W1640261098 modified "2023-09-27" @default.
- W1640261098 title "High Resolution Simulation of Galaxy Formation with Feedback" @default.
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