Fig. 20
PDF of μ1 = cos θ1 similar to that in Fig. 2 for oblate (solid line) and prolate (dashed line) central galaxies, restricted to the intermediate mass range. Tendency to lie orthogonal to the minor axis is stronger for prolate structures, as in this case the minor axis is most often orthogonal to the filament direction and the galactic plane is poorly defined.
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