Jun 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nyasa.596..198t&link_type=abstract
(Galactic models; Proceedings of the 4th Florida Workshop on Nonlinear Dynamics, Gainesville, FL, Mar. 1, 2, 1989. A91-30826 12-
Physics
3
Dynamic Models, Galactic Structure, Ring Galaxies, Galactic Rotation, Oblate Spheroids, Spiral Galaxies
Scientific paper
The geometric properties of the dark halo in polar ring galaxies are studied. The S0 disk is used to define one principal plane of such a galaxy, and the dark halos are investigated in terms of rotation curves, stable and massless rings, transient rings, and self-gravitating rings. Whether polar rings are stable or are transient structures is considered.
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