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DYNAMICS OF GALACTIC SATELLITES ON ELONGATED ORBITS

Current models of galactic satellites assume that the tidal field only imposes a limiting tidal radius to the satellite, without any other effect from that field on the internal dynamics of the satellite (e.g., Binney & Tremaine 1987). An interesting generalization of King’s models, due to Heggie and Ramamani (hereafter HR), replaces the energy integral by the Jacobi integral, thus accounting for some of the effects of the tidal field on the satellite.