Formation of a system of globular clusters in the case of the interaction of a giant E-galaxy with other galaxies

Details Formation of a system of globular clusters in the case of the interaction of a giant E-galaxy with other galaxies Formation of a system of globular clusters in the case of the interaction of a giant E-galaxy with other galaxies

Oct 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kfnt....8...63b&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 8, no. 5, p. 63-71.

Other

Elliptical Galaxies, Galactic Evolution, Globular Clusters, Interacting Galaxies, Astronomical Models, Celestial Mechanics, Three Body Problem

Scientific paper

The formation of the globular cluster system (GCS) of a giant elliptical (gE) galaxy as the result of tidal interactions and merges with other galaxies is investigated. The properties of the proper GCS of a gE galaxy after interaction with several galaxies as well as the properties of the trapped GCS are determined by means of multiple solutions of a restricted three-body problem. The calculated density profiles of the GCS, orbit eccentricities, and velocity dispersions of globular clusters are compared with those observed in gE galaxies.

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