Evolution of Galaxy Clustering

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dc.creatorBagla, J. S.
dc.date1997-09-24
dc.date.accessioned2026-07-07T02:24:18Z
dc.date.available2026-07-07T02:24:18Z
dc.descriptionWe 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.
dc.descriptionFour pages, 1 figure. Contributed talk at `Large Scale Structure: Tracks and Traces' in Potsdam, Sept.15-19
dc.identifierhttps://arxiv.org/abs/astro-ph/9709230
dc.identifierhttp://arxiv.org/abs/astro-ph/9709230
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11568
dc.subjectAstrophysics
dc.titleEvolution of Galaxy Clustering
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