Resolving the structure of cold dark matter halos - Moore, Governato, et al. - 1998 () Citation Context ...rdson et al., 2000; Stadel, 2001; Wadsley et al., 2004) to perform the integrations. This is a parallel,
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Dark Matter (DM) is usually studied in connection with rotational curves in the outskirts of the galaxies. However, the role of DM might be different in th
structure of cold dark matter halos. If the interaction cross section is not exceptionally –5 – large, the dark matter system cannot be treated as a collision dominated, hydrodynamical fluid. Section 2 therefore introduces a new numerical Monte-Carlo-N-body (MCN) method ...
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that the structure and dynamics of dark matter halos, as well as the origin of the connection between the halo and galaxy properties, are to be understood in in terms of a joint evolution of the baryonic and dark components, originating at the epoch of the collapse and formation of the ...
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