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- W2012119171 abstract "We use high-resolution N-body simulations to investigate the formation of virialized halos due to the gravitational collapse of collisionless matter. A variety of formation scenarios are studied, ranging from hierarchical clustering to monolithic radial collapse. The goal of these experiments was to study departures from the universal density profiles recently found to arise in cosmological settings. However, we found that even for models that exhibit quite a different formation history, the density and velocity dispersion profiles of the virialized halos are strikingly similar." @default.
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- W2012119171 title "How Universal Are the Density Profiles of Dark Halos?" @default.
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- W2012119171 doi "https://doi.org/10.1086/307161" @default.
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