Galaxy groups and clusters and their brightest galaxies within the cosmic web

Open Access

Fig. 12.

Cumulative distributions of distances of groups from the nearest filament axis for groups of different luminosity. The line colours correspond to the luminosity classes, as shown in the figure. The vertical lines show the characteristic distances from the nearest filament axis, D_fil = 0.5 Mpc and D_fil = 2.5 Mpc.

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