High-resolution simulations of galaxy formation in a cold dark matter scenario

Details High-resolution simulations of galaxy formation in a cold dark matter scenario High-resolution simulations of galaxy formation in a cold dark matter scenario

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...243..295k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 243, no. 2, March 1991, p. 295-308. Research supported by University of Oxford

Statistics

Computation

49

Computational Astrophysics, Dark Matter, Galactic Evolution, Astronomical Models, Cosmic Gases, Gas Dynamics, Two Dimensional Models

Scientific paper

The results of numerical simulations of galaxy clustering in a two-dimensional model are presented. The simulations permitted better resolution than could be obtained in three-dimensional simulations. A spectrum of initial perturbations corresponding to a cold dark matter model was used. It is found that peaks of the linearized density distribution are not reliable tracers of eventual galaxy distribution.

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