Fig. 12.

dynamical map on the parametric plane Mbar–Rbar showing the stability of the Sun’s orbits as a function of the bar’s mass and radius. The orbits are stable in the light domains and are strongly unstable in the red hatched regions. The parameters adopted in the basic set place the Sun in the position shown by a blue cross symbol. The values of the rest of the parameters are taken from Table 1.
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