Statistics – Computation
Scientific paper
Jul 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...200....5d&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 200, no. 1-2, July 1988, p. 5-8.
Statistics
Computation
12
Elliptical Galaxies, Galactic Clusters, Galactic Evolution, Galactic Structure, Astronomical Models, Computational Astrophysics, Monte Carlo Method
Scientific paper
The authors show that the true axial ratios of clusters of galaxies (of the order of 0.4) are considerably flatter than those of elliptical galaxies. Moreover, the difference between the oblate and prolate spheroidal representation of the real shape of galaxy clusters is not significantly large. The flatness of the clusters seems to favor the Zel'dovich pancake picture for the birth of galaxy clusters.
di Fazio A.
Flin Piotr
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