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Gas in a Cosmological N-Body Simulation

  • P. A. Thomas
  • R. G. Carlberg
Part of the NATO ASI Series book series (ASIC, volume 264)

Abstract

We look at the behaviour of gas in a cosmological n-nody simulation which contains cold dark matter and dissipative gas. The cooling algorithm is chosen so that galaxy formation occurs as in the scheme of Rees & Ostriker (1977). Perturbations of the microwave background radiation are small except through the cores of clusters of galaxies.

Keywords

Phase Diagram Measured Temperature Kinetic Theory Star Formation Particle Interaction 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Copyright information

© Kluwer Academic Publishers 1989

Authors and Affiliations

  • P. A. Thomas
    • 1
  • R. G. Carlberg
    • 1
  1. 1.C.I.T.A.TorontoCanada

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