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...
| Κύριοι συγγραφείς: | , , , , , |
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| Μορφή: | Journal article |
| Έκδοση: |
Cambridge University Press
2016
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