Probing IGM large-scale flows: warps in galaxies at shells of voids
Context: Hydrodynamical cosmological simulations predict flows of the intergalactic medium along the radial vector of the voids, approximately in the direction of the infall of matter at the early stages of the galaxy formation. Aims: These flows might be detected by analysing the dependence of the warp amplitude on the inclination of the galaxies
López-Corredoira, M. et al.
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2008