Substructure and halo density profiles in a Warm Dark Matter scenario
Astrophysics
2007-05-23 v1
Abstract
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.
Keywords
Cite
@article{arxiv.astro-ph/0009317,
title = {Substructure and halo density profiles in a Warm Dark Matter scenario},
author = {P. Colin and V. Avila-Reese and O. Valenzuela},
journal= {arXiv preprint arXiv:astro-ph/0009317},
year = {2007}
}
Comments
2 pages, to appear in "Galaxy Disks and Disk Galaxies," eds. J. G. Funes & E. M. Corsini (ASP Conference Series)