The numerical simulation of evolution of interacting galaxies with the structure of bulge, disk and halo.

Details The numerical simulation of evolution of interacting galaxies with the structure of bulge, disk and halo. The numerical simulation of evolution of interacting galaxies with the structure of bulge, disk and halo.

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994acaps..14..313l&link_type=abstract

Acta Astrophys. Sin., Vol. 14, No. 4, p. 313 - 322

Astronomy and Astrophysics

Astrophysics

Interacting Galaxies: Three-Body Problem, Interacting Galaxies: Numerical Simulations, Interacting Galaxies: Evolution, Disk Galaxies: Galaxy Mergers

Scientific paper

A perfect three-body model is used in the numerical simulation of interacting galaxies for studying whether merging disk galaxies make an elliptical galaxy. It is shown that there are two possibilities: If the angle between disk plane and orbital plane of both galaxies do not equal to zero, it is possible that merging galaxies form an elliptical galaxy. If the angle is equal to zero the merging galaxies will form a new disk galaxy.

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