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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. 14.

Euler characteristic (top panels) and the morphological signature ﹩K_{1}﹩‐﹩K_{2}﹩ (bottom panels) for the empirical models. Left panels: ﹩N_{\mathrm{cl}\,}=25﹩, ﹩N_{\mathrm{gal}\,}=20﹩, and the size of the clusters is 1 and 5 (in grid units), and the combined model where the centers of clusters coincide. Solid line: model CL125; dashed line: model CL525; dot‐dashed line: model CL125525. Middle panels: ﹩N_{\mathrm{cl}\,}=50﹩, ﹩N_{\mathrm{gal}\,}=10﹩, and the size of clusters is 1 and 5 (in grid units), and the combined model where the centers of clusters coincide. Solid line: model CL150; dashed line: model CL550; dot‐dashed line: model CL150550. Right panels: Combined models where the centers do not coincide. "Fil" denotes a simple filament with randomly distributed points. Solid line: model CL125150; dashed line: model CL525150; dot‐dashed line: model "Fil."

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