Arguments in favour of physical reality of the peculiar (200 - 300) MPC scale in the distribution of the rich clusters of galaxies

Details Arguments in favour of physical reality of the peculiar (200 - 300) MPC scale in the distribution of the rich clusters of galaxies Arguments in favour of physical reality of the peculiar (200 - 300) MPC scale in the distribution of the rich clusters of galaxies

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ncimc..12..639k&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 12 C, Sept.-Oct. 1989, p. 639-647.

Astronomy and Astrophysics

Astronomy

Galactic Clusters, Spatial Distribution, Universe, Astronomical Models, Red Shift

Scientific paper

It is necessary to examine the significance of the recently discovered
peak in the spatial two-point correlation function determined for the
rich Abell clusters. The different possible ways to do it are discussed,
and a program of further observations is proposed.

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