Evolution of Galaxy Clustering
Abstract
Description
We show that the galaxy correlation function does not evolve in proportion with the correlation function of the underlying mass distribution. Earliest galaxies cluster very strongly and the amplitude of the galaxy correlation function decreases from this large value. This continues till the average peaks have collapsed, after which, the galaxy correlation function does not evolve very strongly.
Four pages, 1 figure. Contributed talk at `Large Scale Structure: Tracks and Traces' in Potsdam, Sept.15-19
Four pages, 1 figure. Contributed talk at `Large Scale Structure: Tracks and Traces' in Potsdam, Sept.15-19