Fig. 8 from Toward Understanding Rich Superclusters

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Toward Understanding Rich Superclusters

Authors: M. Einasto, E. Saar, V. J. Martínez, J. Einasto, L. J. Liivamägi, E. Tago, J.-L. Starck, V. Müller, P. Heinämäki, P. Nurmi, S. Paredes, M. Gramann, and G. Hütsi

Einasto et al. 2008 The Astrophysical Journal 685 83.

Provider: AAS Journals

Caption: Fig. 8.

Supercluster SCl 9. Top panels: Minkowski functional ﹩V_{3}﹩ (the Euler characteristic) vs. the mass fraction ﹩m_{f}﹩ for bright (B, ﹩M\leq -20.0﹩) and faint (F, ﹩M> -20.0﹩) galaxies (top left), for early‐ and late‐type galaxies (top middle), and for red and blue galaxies (top right). Bottom panels: Morphological signatures ﹩K_{1}﹩ (planarity)–﹩K_{2}﹩ (filamentarity) for the same populations. Symbols as in Fig. 7.

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