Physics
Scientific paper
Nov 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983phlb..131..116c&link_type=abstract
Physics Letters B, Volume 131, Issue 1-3, p. 116-120.
Physics
31
Scientific paper
We have evaluated the probability distribution for finding n galaxies in a Zwicky cluster for six regions of the sky for a depth sample corresponding to 15 × 103 km/s < Vs < 60 × 103 km/s red-shift velocity. Two regions differ from the other four by having a significantly greater high multiplicity tail and a lower peak value. In our view these tails correspond to ongoing gravitational coalescence of clusters, which is more effective in more heterogeneous regions. We obtain by subtraction a distribution to be identified with the original cluster distribution. The form of this distribution belongs to a general class characteristic of chaotic production mechanisms already identified in photoelectron counts from thermal sources and in hadronic charged particle multiplicity distributions. The possible nature of this universal mechanism is discussed.
Carruthers Peter
Duong-van Minh
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