Morphological segregation of galaxies on large scales

Details Morphological segregation of galaxies on large scales Morphological segregation of galaxies on large scales

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991tpsu.rept...75m&link_type=abstract

In MPI für Physik und Astrophysik, Traces of the Primordial Structure in the Universe p 75-83 (SEE N92-29833 20-90)

Mathematics

Logic

Galactic Evolution, Galactic Structure, Galaxies, Galactic Mass, Mass Distribution, Morphology, Positioning, Red Shift

Scientific paper

To test possible morphological segregation of galaxies on large scales, pair count ratio (between early type and late type galaxies) and clustering analysis were used to galaxy redshift samples formed in both supercluster regions and in regions where there is no apparent large concentration of galaxy distribution, and to galaxy samples in which galaxies in clusters and groups of galaxies are removed. It was found that systematic segregation by morphology exists on scales up to approximately 10/h Mpc.

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