Linking Cluster Formation to Large Scale Structure

Details Linking Cluster Formation to Large Scale Structure Linking Cluster Formation to Large Scale Structure

1997-11-05

arxiv.org/abs/astro-ph/9711040v1

Astronomy and Astrophysics

Astrophysics

6 pages (incl. 7 figs)

Scientific paper

We use two high resolution CDM simulations to show that (i) when clusters of galaxies form the infall pattern of matter is not random but shows clear features which are correlated in time; (ii) in addition, the infall patterns are correlated with the cluster's surrounding Large Scale Structure; (iii) Large Scale Structure shows a mix of both filaments and sheets; (iv) the amount of mass in filaments is slightly larger for a low $\Omega$ model.

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