Swirling around filaments: are large-scale structure vortices spinning up dark haloes?
The kinematic analysis of dark matter and hydrodynamical simulations suggests that the vorticity in large-scale structure is mostly confined to, and predominantly aligned with, their filaments, with an excess of probability of 20 per cent to have the angle between vorticity and filaments direction l...
| Main Authors: | , , , , , , , , , , , |
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| Formato: | Journal article |
| Publicado: |
Oxford University Press
2014
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