Substructure and halo density profiles in a Warm Dark Matter scenario

Details Substructure and halo density profiles in a Warm Dark Matter scenario Substructure and halo density profiles in a Warm Dark Matter scenario

2000-09-20

arxiv.org/abs/astro-ph/0009317v1

ASP Conference Series, 230, p. 651-652 (2001)

Astronomy and Astrophysics

Astrophysics

2 pages, to appear in "Galaxy Disks and Disk Galaxies," eds. J. G. Funes & E. M. Corsini (ASP Conference Series)

Scientific paper

High-resolution cosmological N-body simulations were performed in order to
study the substructure of Milky Way-like galactic halos and the density
profiles of halos in a warm dark matter scenario. The results favor this
scenario with respect to the cold dark matter one.

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