The origin of galactic clusters

Details The origin of galactic clusters The origin of galactic clusters

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982s%26w....21..285h&link_type=abstract

Sterne und Weltraum, vol. 21, July-Aug. 1982, p. 285. In German.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Cosmology, Galactic Clusters, Adiabatic Conditions, Gravitational Effects, Mass Distribution, Statistical Analysis, Universe

Scientific paper

The gravitational and adiabatic models of the origin of galactic clusters are compared in the context of a statistical study of cluster distribution. The study found that the clusters tend toward elliptical shape, that neighboring clusters are similarly oriented, that clusters and their brightest members are similarly oriented, and that cluster orientation depends on the cluster distribution in the general neighborhood. The first two findings are compatible with the gravitational model but the latter two are not. The distribution of matter in the universe suggests a bubble structure, each bubble having a diameter of about 100 Mpc.

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