Collisions and relaxation in galaxy clusters

Details Collisions and relaxation in galaxy clusters Collisions and relaxation in galaxy clusters

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasp...87..333n&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 87, Apr. 1975, p. 333, 334.

Astronomy and Astrophysics

Astronomy

Collisions, Cosmology, Galactic Clusters, Interacting Galaxies, Relaxation (Mechanics), Two Body Problem, Celestial Mechanics, Gravitational Effects, Plasma Oscillations, Time Dependence

Scientific paper

The rate of close collisions among galaxies in a cluster, and the rates
of both gravitational two-body and violent relaxation are shown, in most
cases, to be proportional to the Hubble constant. Therefore, the number
of collisions or the degree of relaxation attained in one Hubble time
are invariant to the Hubble constant.

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