Distribution of quasars and formation of large-scale structures

Details Distribution of quasars and formation of large-scale structures Distribution of quasars and formation of large-scale structures

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.115...99f&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 115, no. 1, Oct. 1985, p. 99-106.

Astronomy and Astrophysics

Astrophysics

15

Cosmology, Galactic Clusters, Mass Distribution, Quasars, Lyman Alpha Radiation, Monte Carlo Method, Red Shift

Scientific paper

According to the proposal developed by Fang et al. (1984) on formation of large-scale structure in the Universe, it should be expected that: (1) The distribution of quasars should be different from that of galaxies by no strong inhomogeneity on the scale of 10 - 100 Mpc. (2) The distributions of quasars with Z > 2 and Z < 2 should be different from each other with no large-scale structure in the former case, and conversely in the latter one. The authors' various statistical results obtained from quasar distributions are consistent with these predictions.

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