2 pages, 4 figures, in the 5th International Conference "The Fabulous destiny of galaxies:Bridging past and present", (in press)The dynamical evolution of barred galaxies depends crucially on the fraction and their spacial distribution of chaotic orbits in them. In order to distinguish between the two kinds of orbits, we use the Smaller Alignment Index (SALI) method, a very powerful method which can be applied to problems of galactic dynamics. Using model potentials, and taking into account the full 3D distribution of matter, we discuss how the distribution of chaotic orbits depends on the main model parameters, like the mass of the various components and the bar axial ratio
I summarize the dynamical mechanisms that have been found to shape structures such as the spirals an...
Self-consistent N-body simulations are efficient tools to study galactic dynamics. However, using th...
We establish a dynamical mechanism to explain the origin of the asymmetry between the arms observed ...
2 pages, 4 figures, in the 5th International Conference "The Fabulous destiny of galaxies:Bridging p...
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...
2 pages, 4 figures, in the \"Semaine de lÁstrophysique Francaise Journees de la SF2A\", (in press)A ...
8 pages, 3 figures, to appear in the proceedings of the international conference "Chaos in Astronomy...
Studies of dynamical stability (chaotic versus regular motion) in galactic dynamics often rely on st...
This paper aims to verify the influence of the bar, its pattern speed (Omega(b)) and its rate of gro...
We explore the regular or chaotic nature of orbits of stars moving in the meridional (R, z) plane of...
24 pages, 11 figures, invited review, 2004 DDA meeting in Cannes, april 19-23, Celestial Mechanics &...
Aims. The distinction between regular and chaotic motion in galaxies is undoubtedly an iss...
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...
I summarize the dynamical mechanisms that have been found to shape structures such as the spirals an...
Self-consistent N-body simulations are efficient tools to study galactic dynamics. However, using th...
We establish a dynamical mechanism to explain the origin of the asymmetry between the arms observed ...
2 pages, 4 figures, in the 5th International Conference "The Fabulous destiny of galaxies:Bridging p...
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...
2 pages, 4 figures, in the \"Semaine de lÁstrophysique Francaise Journees de la SF2A\", (in press)A ...
8 pages, 3 figures, to appear in the proceedings of the international conference "Chaos in Astronomy...
Studies of dynamical stability (chaotic versus regular motion) in galactic dynamics often rely on st...
This paper aims to verify the influence of the bar, its pattern speed (Omega(b)) and its rate of gro...
We explore the regular or chaotic nature of orbits of stars moving in the meridional (R, z) plane of...
24 pages, 11 figures, invited review, 2004 DDA meeting in Cannes, april 19-23, Celestial Mechanics &...
Aims. The distinction between regular and chaotic motion in galaxies is undoubtedly an iss...
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...
I summarize the dynamical mechanisms that have been found to shape structures such as the spirals an...
Self-consistent N-body simulations are efficient tools to study galactic dynamics. However, using th...
We establish a dynamical mechanism to explain the origin of the asymmetry between the arms observed ...