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- W2110854340 abstract "To understand cluster formation and evolution it is important to understand the evolution of cluster substructure. The work described here focuses upon a set of fully self-consistent numerical simulations within a CDM cosmology. Within the simulations we follow in detail the temporal and spatial properties of individually tracked satellite galaxies. The host galaxy clusters were chosen to sample a variety of formation histories, ages, and triaxialities. Despite their obvious differences, we find striking similarities within the associated substructure populations. Namely, the satellite galaxy orbital distributions are indistinguishable between the galaxy clusters.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html" @default.
- W2110854340 created "2016-06-24" @default.
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- W2110854340 date "2004-03-01" @default.
- W2110854340 modified "2023-10-16" @default.
- W2110854340 title "The dynamics of cluster substructure" @default.
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- W2110854340 doi "https://doi.org/10.1017/s1743921304000596" @default.
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