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Nonlinear Stochastic Biasing of Galaxies and Dark Halos in Cosmological Hydrodynamic Simulations

  • Authors: Kohji Yoshikawa, Atsushi Taruya, Y. P. Jing, and Yasushi Suto

Yoshikawa et al. 2001 The Astrophysical Journal 558 520.

  • Provider: AAS Journals

Caption: Fig. 4.

Snapshots of the most massive cluster (﹩M\simeq 8\times 10^{14}\,M_{\odot }﹩) in the simulation at ﹩z=0﹩. Upper left, dark matter; upper right, gas particles; lower left, DM cores; lower right, cold gas. Circles in lower panels indicate the positions of galaxies identified according to our criteria. The comoving size of the box is 6.25 h−1Mpc per side.

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