Typical scales in the large-scale structures of the universe.

Details Typical scales in the large-scale structures of the universe. Typical scales in the large-scale structures of the universe.

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pbeio..23...10d&link_type=abstract

Publications of the Beijing Astronomical Observatory, No. 23, p. 10 - 25

Astronomy and Astrophysics

Astronomy

Universe: Large-Scale Structure, Universe: Galaxy Formation

Scientific paper

Analyses by two-point correlation function and correlation fractal dimension have provided evidences on that the large-scale structure of the universe is neither a simply fractal nor a distribution with power law two-point correlation function exactly. It is shown from the analyses of galaxies, clusters of galaxies and quasars etc. that typical scales may exist in the large-scale structure of the universe. Existence of the typical scales implies that the formation and evolution of galaxies can not be a pure gravitational process.

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