Secondary peak in clusters of galaxies - A clue to their formation

Details Secondary peak in clusters of galaxies - A clue to their formation Secondary peak in clusters of galaxies - A clue to their formation

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....85..154d&link_type=abstract

Astronomy and Astrophysics, vol. 85, no. 1-2, May 1980, p. 154-160.

Astronomy and Astrophysics

Astrophysics

17

Astronomical Models, Cosmology, Galactic Clusters, Adiabatic Conditions, Correlation, Galactic Evolution, Galactic Structure, Line Spectra, Many Body Problem, Perturbation Theory

Scientific paper

A model describing the second peak in clusters of galaxies is suggested.
The secondary shell is assumed to be the natural outcome of the presence
of a cutoff at a damping-scale in the spectrum of linear adiabatic
density perturbations, which induces 'wiggly' spatial correlations on
emergence from a recombination epoch.

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