Time-dependent axisymmetric galactic models

Details Time-dependent axisymmetric galactic models Time-dependent axisymmetric galactic models

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...235...85s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 235, no. 1-2, Aug. 1990, p. 85-93.

Statistics

Computation

4

Astronomical Models, Galactic Structure, Milky Way Galaxy, Stellar Motions, Boltzmann Transport Equation, Computational Astrophysics, Dynamic Models, Galactic Rotation, Many Body Problem, Space-Time Functions, Stellar Orbits, Time Dependence

Scientific paper

The Chandrasekhar theory for the study of the dynamics of stellar motions has been used to derive integrable time-dependent models of collisionless rotating stellar systems. Time-depending potentials are obtained with three isolating integrals in involution. Space and time coordinates can be transformed so that the potentials take a steady-state form whose classification of stellar orbits is already known.

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