We created a self-consistent triaxial stellar system through the cold disipationless collapse of 100,000 particles whose evolution was followed with a multipolar code. The resulting system rotates slowly even though its total angular momentum is zero, i.e., it offers an example of figure rotation. The potential of the system was subsequently approximated with interpolating formulae yielding a smooth potential stationary in the rotating frame. The Lyapunov exponents could then be computed for a randomly selected sample of 3,472 of the bodies that make up the system, allowing the recognition of regular and partially and fully chaotic orbits. The regular orbits were Fourier analyzed and classified using their locations on the frequency map. A ...
We used the N-body code of Hernquist & Ostriker to build a dozen cuspy (γ ≃ 1) triaxial models of st...
We used the N-body code of Hernquist & Ostriker to build a dozen cuspy (γ ≃ 1) triaxial models of st...
In several previous investigations, we presented models of triaxial stellar systems, both cuspy and ...
We created a self-consistent triaxial stellar system through the cold disipationless collapse of 100...
We created a triaxial stellar system through the cold dissipationless collapse of 100,000 particles ...
We used a multipolar code to create, through the dissipationless collapses of systems of 1,000,000 p...
We built two self--consistent models of triaxial, cuspy, rotating stellar systemsadding rotation to ...
We used the N-body code ofWe used the N–body code of Hernquist & Ostriker (1992) to build a dozen cu...
Here I review recent work, by other authors and by myself, on some particular topics related to the ...
We built two self-consistent models of triaxial, cuspy, rotating stellar systems adding rotation to ...
International audienceCelestial bodies approximated with rigid triaxial ellipsoids in a two-body sys...
International audienceCelestial bodies approximated with rigid triaxial ellipsoids in a two-body sys...
International audienceCelestial bodies approximated with rigid triaxial ellipsoids in a two-body sys...
none3noThe gravitational potentials of realistic galaxy models are in general non-integrable, in the...
We used the N-body code of Hernquist & Ostriker to build a dozen cuspy (γ ≃ 1) triaxial models of st...
We used the N-body code of Hernquist & Ostriker to build a dozen cuspy (γ ≃ 1) triaxial models of st...
We used the N-body code of Hernquist & Ostriker to build a dozen cuspy (γ ≃ 1) triaxial models of st...
In several previous investigations, we presented models of triaxial stellar systems, both cuspy and ...
We created a self-consistent triaxial stellar system through the cold disipationless collapse of 100...
We created a triaxial stellar system through the cold dissipationless collapse of 100,000 particles ...
We used a multipolar code to create, through the dissipationless collapses of systems of 1,000,000 p...
We built two self--consistent models of triaxial, cuspy, rotating stellar systemsadding rotation to ...
We used the N-body code ofWe used the N–body code of Hernquist & Ostriker (1992) to build a dozen cu...
Here I review recent work, by other authors and by myself, on some particular topics related to the ...
We built two self-consistent models of triaxial, cuspy, rotating stellar systems adding rotation to ...
International audienceCelestial bodies approximated with rigid triaxial ellipsoids in a two-body sys...
International audienceCelestial bodies approximated with rigid triaxial ellipsoids in a two-body sys...
International audienceCelestial bodies approximated with rigid triaxial ellipsoids in a two-body sys...
none3noThe gravitational potentials of realistic galaxy models are in general non-integrable, in the...
We used the N-body code of Hernquist & Ostriker to build a dozen cuspy (γ ≃ 1) triaxial models of st...
We used the N-body code of Hernquist & Ostriker to build a dozen cuspy (γ ≃ 1) triaxial models of st...
We used the N-body code of Hernquist & Ostriker to build a dozen cuspy (γ ≃ 1) triaxial models of st...
In several previous investigations, we presented models of triaxial stellar systems, both cuspy and ...