Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002mnras.337.1233r&link_type=abstract
Monthly Notice of the Royal Astronomical Society, Volume 337, Issue 4, pp. 1233-1244.
Astronomy and Astrophysics
Astronomy
23
Galaxies: Evolution, Galaxies: Fundamental Parameters, Galaxies: Kinematics And Dynamics, Galaxies: Spiral, Galaxies: Structure
Scientific paper
We have studied the formation of complex central structures in barred galaxies - nested bars, nuclear spirals and circumnuclear rings - by making N-body simulations, which include the gas component as inelastically colliding particles. Our models suggest that many of the observed features in both the stellar and gas components can be explained by the dynamical effect of two or more modes in the stellar disc. Especially, many morphological features in our simulations correspond to analytically studied orbit loops in double-barred potentials. Interestingly, a fast-rotating secondary bar forms in a purely stellar disc in our simulations, which disagrees with some previous studies where the presence of a dissipative component was needed.
Laurikainen Eija
Rautiainen Pertti
Salo Heikki
No associations
LandOfFree
Simulations of central structure in barred galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Simulations of central structure in barred galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Simulations of central structure in barred galaxies will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1159247