A numerical simulation of galaxy subcluster mergers

Details A numerical simulation of galaxy subcluster mergers A numerical simulation of galaxy subcluster mergers

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993egte.conf..263r&link_type=abstract

In NASA. Ames Research Center, The Evolution of Galaxies and Their Environment p 263-264 (SEE N93-26706 10-90)

Astronomy and Astrophysics

Astronomy

1

Astronomical Models, Galactic Clusters, Galactic Evolution, Interacting Galaxies, Three Dimensional Models, Cosmic Gases, Dark Matter, Intergalactic Media, Many Body Problem, Morphology, Velocity Distribution, X Rays

Scientific paper

We present preliminary results of a 3-D numerical simulation of two
merging subclusters of galaxies. By self-consistently modelling the
intracluster gas and dark matter dynamics, we hope to gain insight as to
how the dynamics of both relate to such observables as the cluster x-ray
emission, radio source morphology, and velocity dispersions.

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