The existence of the structural anisotropy of the Jagiellonian field of the galaxies

Details The existence of the structural anisotropy of the Jagiellonian field of the galaxies The existence of the structural anisotropy of the Jagiellonian field of the galaxies

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.185..223g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 185, no. 2, Nov. 1991, p. 223-235.

Astronomy and Astrophysics

Astrophysics

Astronomical Catalogs, Galactic Clusters, Galactic Structure, Anisotropy, Error Analysis, Histograms, Statistical Analysis

Scientific paper

The cluster-analysis method is used to investigate the Jagiellonian field of galaxies from the standpoint of the existence of the structural anisotropy. The position angle of the major axis and the ratio of axes of the effective ellipse of inertness are calculated for every cluster. The possible space scale of anisotropy is discussed; its lower limit is estimated at a magnitude of 500 Mps.

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