Why do galactic spins flip in the cosmic web? A Theory of Tidal Torques near saddles

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...

書目詳細資料
Main Authors:	Pichon, C, Codis, S, Pogosyan, D, Dubois, Y, Desjacques, V, Devriendt, J
格式:	Journal article
出版:	Cambridge University Press 2016

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