We extend recent investigations on the integrability of oblique orbits of t
est particles under the gravitational field corresponding to the superposit
ion of an infinitesimally thin disk and a monopole to the more realistic ca
se, for astrophysical purposes, of a thick disk. Exhaustive numerical analy
ses were performed and the robustness of the recent results is confirmed. W
e also found that, for smooth distributions of matter, the disk thickness c
an attenuate the chaotic behavior of the bounded oblique orbits. Perturbati
ons leading to the breakdown of the reflection symmetry about the equatoria
l plane, nevertheless, may enhance significantly the chaotic behavior, in a
greement with recent studies on oblate models. (C) 2000 Elsevier Science B.
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