The problem of a Klein-Gordon particle moving in equal vector and scalar Rosen-Morse-type potentials is solved in the framework of Feynman's path integral approach. Explicit path integration leads to a closed form for the radial Green's function associated with different shapes of the potentials. For q ≤ −1, and 1 2α ln |q| < r < +∞, the energy equation and the corresponding wave functions are deduced for the l states using an appropriate approximation to the centrifugal potential term. When −1 < q < 0 or q > 0, it is shown that the quantization conditions for the bound state energy levels En r are transcendental equations which can be solved numerically. Three special cases such as the standard radial Manning-Rosen potential (|q| = 1), the standard radial Rosen-Morse potential (V2 → −V2, q = 1) and the radial Eckart potential (V1 → −V1, q = 1) are also briefly discussed.