1997/09/24 by J. S. Bagla, Bagla, J. S.
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9709230
Four pages, 1 figure. Contributed talk at `Large Scale Structure: Tracks and Traces' in Potsdam, Sept.15-19
arxiv created 1997/09/24 · arxiv updated 2009/12/01
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.