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This paper is a continuation of our recent paper devoted to refining theparameters of three component (bulge, disk, halo) axisymmetric model Galacticgravitational potentials differing by the expression for the dark matter halousing the velocities of distant objects. In all models the bulge and diskpotentials are described by the Miyamoto-Nagai expressions. In our previouspaper we used the Allen-Santill'an (I), Wilkinson--Evans (II), andNavarro-Frenk-White (III) models to describe the halo. In this paper we use aspherical logarithmic Binney potential (model IV), a Plummer sphere (model V),and a Hernquist potential (model VI) to describe the halo. A set of present-dayobservational data in the range of Galactocentric distances R from 0 to 200 kpcis used to refine the parameters of the listed models, which are employed mostcommonly at present. The model rotation curves are fitted to the observedvelocities by taking into account the constraints on the local matter densityand the vertical force . Model VI looks best among the three models consideredhere from the viewpoint of the achieved accuracy of fitting the model rotationcurves to the measurements. This model is close to the Navarro-Frenk-Whitemodel III refined and considered best in our previous paper, which is shownusing the integration of the orbits of two globular clusters, Lynga 7 and NGC5053, as an example.

Parameters of Three Selected Model Galactic Potentials Based on the Velocities of Objects at Distances up to 200 kpc