Abstract
The effect of an oscillating massive particle on the motion of stars in a spherical Plummer gravitational system is examined for chaotic behaviour for ratios of satellite to parent galaxy masses ranging from .001 to .15. Thee-folding times for chaos are calculated for non-zero angular momentum orbits and discussed in relation to the time-scales for dynamical friction.
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Stewart, P. Galactic chaos driven by an oscillating massive particle. Astrophys Space Sci 234, 63–68 (1995). https://doi.org/10.1007/BF00627283
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DOI: https://doi.org/10.1007/BF00627283