N-body Simulations of Resonance Rings

Details N-body Simulations of Resonance Rings N-body Simulations of Resonance Rings

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..275..169r&link_type=abstract

Disks of Galaxies: Kinematics, Dynamics and Peturbations, ASP Conference Proceedings, Vol. 275. Edited by E. Athanassoula, A. Bo

Astronomy and Astrophysics

Astronomy

Scientific paper

We have made N-body simulations of ring formation in disk galaxies. The
rings are related to resonances, which are induced by rotating stellar
bars and/or spiral arms. Presence of several modes with different
pattern speeds does not inhibit the formation of a ring, but can cause
cyclic evolution in its shape and orientation.

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