N-body simulations of the evolution of clusters of galaxies

Details N-body simulations of the evolution of clusters of galaxies N-body simulations of the evolution of clusters of galaxies

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991tpsu.rept..153s&link_type=abstract

In MPI für Physik und Astrophysik, Traces of the Primordial Structure in the Universe p 153-160 (SEE N92-29833 20-90)

Astronomy and Astrophysics

Astrophysics

Astronomical Models, Galactic Clusters, Galactic Evolution, Cosmology, Simulation

Scientific paper

Several models for the formation of clusters of galaxies with different initial conditions are presented: spherical collapse models, a steady infall model and a collision model. For each of these models the evolution and the phase space distribution of the virialized state was investigated. It is shown that the phase space distribution in the virial equilibrium still contains information on the different types of initial conditions.

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