Physics
Scientific paper
May 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985sssmp..28..517f&link_type=abstract
Scientia Sinica, Series A - Mathematical, Physical, Astronomical and Technical Sciences (ISSN 0253-5831), vol. 28, May 1985, p.
Physics
Cosmic Rays, Cosmology, Dark Matter, Galactic Clusters, Matter (Physics), Quasars, Star Clusters, Globular Clusters, Histograms, Monte Carlo Method, Relic Radiation
Scientific paper
According to the scenario, developed in the previous paper, on the formation of large scale structure in the universe, it would be expected that: (1) the distribution of quasars should differ from that of galaxies because it has no strong inhomogeneity on the scale of 10-100 Mpc; (2) the distributions of quasars with Z greater than 2 and Z less than 2 should differ from each other because of the absence of large structure in the former but its presence in the latter. Various analyses on quasar distribution are consistent with these predictions. Particularly, the nearest neighbor test for the complete quasar sample given by Savage and Bolton (1979) clearly shows that the distribution of Z greater than 2 quasars is rather homogeneous while the Z less than 2 quasars have a tendency to clustering.
Chu Yan-Yi
Fang Lujun
Zhu Xiyu
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