Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...326..493p&link_type=abstract
Astronomy and Astrophysics, v.326, p.493-500
Astronomy and Astrophysics
Astrophysics
13
Galaxies: Kinematics And Dynamics
Scientific paper
We apply the method of dynamical spectra in the case of a barred galaxy potential. We show its efficiency in detecting tiny ordered domains embedded in big chaotic seas. We can separate ordered from chaotic domains in the corotation region by integrating a number of orbits only for 10-20 orbital periods each. The method is more efficient than the use of the Poincare section, while other methods require a much longer time. Our method of separation between ordered and chaotic orbits is useful when attacking the self-consistency problem in the corotation region of galaxies. Then we describe the differences between the dynamical spectra of orbits in a transition region from ordered to chaotic.
Contopoulos George
Efthymiopoulos Ch.
Patsis Panos A.
Voglis Nikos
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