Analysis of the large scale structure from samples given by quasi-one-dimensional redshift survey

Details Analysis of the large scale structure from samples given by quasi-one-dimensional redshift survey Analysis of the large scale structure from samples given by quasi-one-dimensional redshift survey

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acaps..11..306d&link_type=abstract

(Acta Astrophysica Sinica, vol. 11, no. 4, 1991, p. 306-310) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 16, no. 1

Astronomy and Astrophysics

Astronomy

Galactic Structure, Red Shift, Sky Surveys (Astronomy), Galactic Clusters, Spatial Distribution

Scientific paper

Large scale structure in the distribution of galaxies is investigated by analyzing samples taken from a complete redshift survey in five pencil-beam fields and a sparse redshift survey in nine pencil-beam fields. Fractal dimension in the distributions are calculated by a revised method. The results show that distribution of galaxies in these samples do have typical scale which is about 3-4.5/h Mpc. It is consistent with that obtained by Shanks et al.

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