Why do galactic spins flip in the cosmic web? A Theory of Tidal Torques near saddles
Filaments of the cosmic web drive spin acquisition of disc galaxies. The point process of filament-type saddle represent best this environment and can be used to revisit the Tidal Torque Theory in the context of an anisotropic peak (saddle) background split. The constrained misalignment between the...
| 主要な著者: | , , , , , |
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| フォーマット: | Journal article |
| 出版事項: |
Cambridge University Press
2016
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