Deep galactic surveys and the structure of the universe

Details Deep galactic surveys and the structure of the universe Deep galactic surveys and the structure of the universe

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...383...41b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 383, Dec. 10, 1991, p. 41-50.

Computer Science

Numerical Analysis

13

Cosmology, Deep Space, Galactic Clusters, Mathematical Models, Numerical Analysis, Poisson Equation, Voids

Scientific paper

A new method of analysis of deep galactic surveys is presented and applied to the available data. A few model distributions are considered, indicating that the one-dimensional distribution of elements of the large-scale structure (LSS) in the regions between voids is almost Poissonian and to estimate its parameters. The typical size of voids is also estimated. The reality of the super LSS (of an approximate size of 80/h Mpc) which probably is connected with the existence of population of large voids is confirmed. This result is also supported by an analysis of distribution of the C IV doublets in absorption spectra of quasars.

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