Dynamics and morphology of galactic mergers.

Details Dynamics and morphology of galactic mergers. Dynamics and morphology of galactic mergers.

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ncima.108.1207c&link_type=abstract

Nuovo Cimento A, Vol. 108A, No. 10, p. 1207 - 1222

Computer Science

Numerical Analysis

Galaxy Mergers: Dynamics, Galaxy Mergers: Morphology, Elliptical Galaxies: N-Body Simulations

Scientific paper

In a N-body simulation of a non-dissipative collapse, the spin parameters of the final outcome of evolution took values comparable with those of a sample of elliptical galaxies deduced from observations. The authors make a numerical analysis of the merging of a disk-like structure with an initially spheroidal configuration with the purpose of studying the morphological properties and the angular-momentum distribution of the mergers and compare these results with the properties of the structures which were generated by collapse.

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