The orbital structure of galactic halos

Details The orbital structure of galactic halos The orbital structure of galactic halos

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...384..491l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 384, Jan. 10, 1992, p. 491-501.

Astronomy and Astrophysics

Astrophysics

42

Celestial Mechanics, Galactic Rotation, Halos, Stellar Motions, Stellar Orbits, Astronomical Models, Orbit Perturbation

Scientific paper

Numerical experiments have been carried out to investigate the restrictions on triaxial models for the halos of galaxies. Some of the conclusions drawn from the numerical experiments are: (1) the dominant occurrence of boxlets may be a fairly general phenomenon in triaxial galactic halos; (2) most of the tube orbits in the halo are not affected by the higher resonances; and (3) triaxiality truncations favor the existence of self-consistent equilibria in galactic halos.

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