Astronomy and Astrophysics – Astronomy
Scientific paper
May 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.244..322r&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 244, May 15, 1990, p. 322-327.
Astronomy and Astrophysics
Astronomy
2
Evolution (Development), Galactic Clusters, Globular Clusters, Universe, Astronomical Models, Brightness Distribution, Galactic Mass, Radial Distribution
Scientific paper
The dynamical evolution of globular cluster systems of galaxies that belong to clusters of galaxies was followed during an interval similar to the age of the universe. Tidal stripping and accretion effects were investigated, grouping the galaxies in radial distance bins according to two different criteria: (1) their final positions after 10 Gyr of dynamical evolution, and (2) their time-averaged radial distances over the same interval. The results obtained from the two different samples are essentially the same, and in both cases it clearly turns out that galaxies in the central region of a cluster are strongly affected, while galaxies outside that region suffer only small effects.
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