2 pages, 4 figures, in the \"Semaine de lÁstrophysique Francaise Journees de la SF2A\", (in press)A very important issue in the area of galactic dynamics is the detection of chaotic and ordered motion inside galaxies. In order to achieve this target, we use the Smaller ALignment Index (SALI) method, which is a very suitable tool for this kind of problems. Here, we apply this index to 3D barred galaxy potentials and we present some results on the chaotic behavior of the model when its main parameters vary
We study the behavior of orbits in a barred galaxy model composed of an harmonic oscillator potentia...
International audienceWe investigate the evolution of phase space close to complex unstable periodic...
Some 30 % of disc galaxies have a pronounced central bar feature in the disc plane and many more hav...
2 pages, 4 figures, in the \"Semaine de lÁstrophysique Francaise Journees de la SF2A\", (in press)A ...
International audienceThe dynamical evolution of barred galaxies depends crucially on the fraction a...
7 pages, 3 figures, in the 7th Astronomy Conference of the Hellenic Astronomical Society, Kefallinia...
International audienceThe distinction between the chaotic and regular behaviour of orbits in galacti...
8 pages, 3 figures, to appear in the proceedings of the international conference "Chaos in Astronomy...
Abstract. We apply the method of the Smaller Alignment Index (SALI) for determining the ordered or c...
Studies of dynamical stability (chaotic versus regular motion) in galactic dynamics often rely on st...
We study the regular or chaotic nature of orbits in a 3D potential describing a triaxial galaxy surr...
The ordered or chaotic character of orbits of stars moving in the meridional (R, z) plane of an anal...
Aims. The distinction between regular and chaotic motion in galaxies is undoubtedly an iss...
A study of the dynamical characteristics of the phase space corresponding to the vibrations of the L...
This paper aims to verify the influence of the bar, its pattern speed (Omega(b)) and its rate of gro...
We study the behavior of orbits in a barred galaxy model composed of an harmonic oscillator potentia...
International audienceWe investigate the evolution of phase space close to complex unstable periodic...
Some 30 % of disc galaxies have a pronounced central bar feature in the disc plane and many more hav...
2 pages, 4 figures, in the \"Semaine de lÁstrophysique Francaise Journees de la SF2A\", (in press)A ...
International audienceThe dynamical evolution of barred galaxies depends crucially on the fraction a...
7 pages, 3 figures, in the 7th Astronomy Conference of the Hellenic Astronomical Society, Kefallinia...
International audienceThe distinction between the chaotic and regular behaviour of orbits in galacti...
8 pages, 3 figures, to appear in the proceedings of the international conference "Chaos in Astronomy...
Abstract. We apply the method of the Smaller Alignment Index (SALI) for determining the ordered or c...
Studies of dynamical stability (chaotic versus regular motion) in galactic dynamics often rely on st...
We study the regular or chaotic nature of orbits in a 3D potential describing a triaxial galaxy surr...
The ordered or chaotic character of orbits of stars moving in the meridional (R, z) plane of an anal...
Aims. The distinction between regular and chaotic motion in galaxies is undoubtedly an iss...
A study of the dynamical characteristics of the phase space corresponding to the vibrations of the L...
This paper aims to verify the influence of the bar, its pattern speed (Omega(b)) and its rate of gro...
We study the behavior of orbits in a barred galaxy model composed of an harmonic oscillator potentia...
International audienceWe investigate the evolution of phase space close to complex unstable periodic...
Some 30 % of disc galaxies have a pronounced central bar feature in the disc plane and many more hav...