This talk summarises several different lines of argument suggesting that one should not expect cuspy nonaxisymmetric galaxies to exist as robust, long-lived collisionless equilibria, i.e., that such objects should not be idealised as time-independent solutions to the collisionless Boltzmann equation
How elliptical galaxy dynamics relate to galaxy structure, stellar populations, spiral galaxies and ...
Cuspy triaxial potentials admit a large number of chaotic orbits, which moreover exhibit extreme \st...
Here I review recent work, by other authors and by myself, on some particular topics related to the ...
The paper examines whether elliptical galaxies can be considered equilibrium systems in which the gr...
The shape of a cusped galactic nucleus is constrained by the range of shapes of orbits in its gravit...
N-body simulations of collisionless collapse have offered important clues to the construction of rea...
Recent results on chaos in triaxial galaxy models are reviewed. Central mass concentrations like tho...
This talk provides a progress report on an extended collaboration which has aimed to address two bas...
A review of elliptical galaxy dynamics, with a focus on nonintegrable models. Topics covered include...
Elliptical galaxies are modeled as homeoidally striated Jacobi ellipsoids (Caimmi and Marmo 2005) wh...
Elliptical galaxies are modelled as homeoidally striated Jacobi ellipsoids (Caimmi and Marmo 2005) w...
Models of ecological communities that incorporate mutation and spatial dispersal can yield results t...
Schwarzschild models of a Plummer sphere were constructed and compared with analytical results to te...
The modified Newtonian dynamics (MOND), suggested by Milgrom as an alternative to dark matter, impli...
It is suggested that elliptical galaxies are formed in an expansion from a steady-state situation in...
How elliptical galaxy dynamics relate to galaxy structure, stellar populations, spiral galaxies and ...
Cuspy triaxial potentials admit a large number of chaotic orbits, which moreover exhibit extreme \st...
Here I review recent work, by other authors and by myself, on some particular topics related to the ...
The paper examines whether elliptical galaxies can be considered equilibrium systems in which the gr...
The shape of a cusped galactic nucleus is constrained by the range of shapes of orbits in its gravit...
N-body simulations of collisionless collapse have offered important clues to the construction of rea...
Recent results on chaos in triaxial galaxy models are reviewed. Central mass concentrations like tho...
This talk provides a progress report on an extended collaboration which has aimed to address two bas...
A review of elliptical galaxy dynamics, with a focus on nonintegrable models. Topics covered include...
Elliptical galaxies are modeled as homeoidally striated Jacobi ellipsoids (Caimmi and Marmo 2005) wh...
Elliptical galaxies are modelled as homeoidally striated Jacobi ellipsoids (Caimmi and Marmo 2005) w...
Models of ecological communities that incorporate mutation and spatial dispersal can yield results t...
Schwarzschild models of a Plummer sphere were constructed and compared with analytical results to te...
The modified Newtonian dynamics (MOND), suggested by Milgrom as an alternative to dark matter, impli...
It is suggested that elliptical galaxies are formed in an expansion from a steady-state situation in...
How elliptical galaxy dynamics relate to galaxy structure, stellar populations, spiral galaxies and ...
Cuspy triaxial potentials admit a large number of chaotic orbits, which moreover exhibit extreme \st...
Here I review recent work, by other authors and by myself, on some particular topics related to the ...