Back to Volume
Paper: Substructure and Halo Density Profiles in a Warm Dark Matter Cosmology
Volume: 230, Galaxy Disks and Disk Galaxies
Page: 651
Authors: ColĂ­n, P.; Avila-Reese, V.; Valenzuela, O.
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 WDM scenario. The results favor this scenario with respect to the CDM one.
Back to Volume