What determines the morphological fractions in clusters of galaxies?

Details What determines the morphological fractions in clusters of galaxies? What determines the morphological fractions in clusters of galaxies?

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993egte.conf...44w&link_type=abstract

In NASA. Ames Research Center, The Evolution of Galaxies and Their Environment p 44-45 (SEE N93-26706 10-90)

Computer Science

Elliptical Galaxies, Galactic Clusters, Galactic Evolution, Irregular Galaxies, Spiral Galaxies, Statistical Correlation, Morphology, Radii

Scientific paper

A reexamination of Dressler's (1980) sample of nearly 6000 galaxies in 55 clusters shows that the morphology-clustercentric radius relation is more fundamental than the morphology-local density relation. This conclusion is supported by improved correlations when the projected clustercentric radius is used as the independent parameter, and by a comparison of galaxies with the same normalized clustercentric radii by different values of the projected local density.

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