The shape of dark matter haloes in the Aquarius simulations: Evolution and memory
We use the high resolution cosmological N-body simulations from the Aquarius project to investigate in detail the mechanisms that determine the shape of Milky Way-type dark matter haloes. We find that, when measured at the instantaneous virial radius, the shape of individual haloes changes with time...
Main Authors: | , , |
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Format: | Article |
Language: | English |
Published: |
EDP Sciences
2012-02-01
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Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/20121901009 |