The limits are a complicated function of the inclination and eccentricity, but in general, prograde orbits with semi-major axes up to 0.47 rH (Hill sphere radius) can be stable, whereas for retrograde orbits stability can extend out to 0.67 rH.
The limits of stability for orbits are determined by inclination and eccentricity, with prograde orbits being more likely to be stable within a certain range (up to 0.47 times the Hill sphere radius) compared to retrograde orbits which can extend further out (up to 0.67 times the Hill sphere radius).