Substructure and halo density profiles in a Warm Dark Matter scenario

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dc.creatorColin, P.
dc.creatorAvila-Reese, V.
dc.creatorValenzuela, O.
dc.date2000-09-20
dc.date.accessioned2026-07-07T01:55:32Z
dc.date.available2026-07-07T01:55:32Z
dc.descriptionHigh-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.
dc.description2 pages, to appear in "Galaxy Disks and Disk Galaxies," eds. J. G. Funes & E. M. Corsini (ASP Conference Series)
dc.identifierhttps://arxiv.org/abs/astro-ph/0009317
dc.identifierhttp://arxiv.org/abs/astro-ph/0009317
dc.identifierASP Conference Series, 230, p. 651-652 (2001)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1689
dc.subjectAstrophysics
dc.titleSubstructure and halo density profiles in a Warm Dark Matter scenario
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