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Are two of the Neptune Trojans dynamically unstable?

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Figure

Table 1: The best-fit orbits of the eight known Neptune Trojans, taken from the AstDys orbital database on 19th October 2011
Table 2: The orbital elements, along with their associated 1σ uncertainties, of the nominal best-fit orbit for 2001 QR322 as obtained from [33] on 26th January 2009
Figure 1: The decay of the population of clones of 2001 QR322 as a function of time.
Figure 2: The dynamical stability of 2001 QR322 as a function of its initial semi-major axis and eccentricity
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