The inner structure of ΛCDM halos
We have used high resolution N-body simulations to investigate the internal properties of Cold Dark Matter (CDM) halos with virial masses of M(_200) ~ 10(^10) M(_o) at z = 0, comparable to those of dwarf galaxy halos, forming in the ACDM cosmology. In particular, we have focused on providing accurat...
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Durham University
2003
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.399902 |