The existence and stability under linear perturbation of closed timelike curves in the spacetime associated to Schwarzschild black hole pierced by a spinning string are studied. Due to the superposition of the black hole, we find that the spinning string spacetime is deformed in such a way to allow the existence of closed timelike geodesics. The existance of closed timelike curves (CTCs) in the Gödel universe and other apacetimes is a worrying fact since these curves show a clear violation of causality. In some cases these CTCs can be disregarded by energy considerations. Their existance requires an external force acting along the whole CTC, process that may consume a great amount of energy. The energy needed to travel along a CTC in Gödel's universe is computed in [1]. When the external force is null the energy needed to travel is also null. Therefore, in principle, the existence of closed timelike geodesics (CTGs) presents a bigger problem of breakdown of causality.The classical problem of the existence of closed geodesics in Riemannian geometry was solved by Hadamard [2] in two dimensions and by Cartan [3] in an arbitrary number of dimensions. As a topological problem, the existence of CTGs was proved by Tipler [4] in a class of four-dimensional compact Lorentz manifolds with covering space containing a compact Cauchy surface. In a compact pseudo-Riemaniann manifold with Lorentzian signature (Lorentzian manifold) Galloway [5] found sufficient conditions to have CTGs, see also [6].To the best of our knowledge there are four solution to the Einstein equations generated by matter with positive mass density that contain CTGs: a) Soares [7] found a class of cosmological models, solutions of EinsteinMaxwell equations, with a subclass where the timelike paths of matter are closed. For these models the existence of CTGs is demonstrated and explicit examples are given. These CTGs are not linearly stable [8]. b) Steadman [9] described the behavior of CTGs in a vacuum exterior for the van Stockum solution that represents an infinite rotating dust cylinder. For this solution explicit examples of CTCs and CTGs are shown. There are stable CTGs in this spacetime [8]. c) Bonnor and Steadman [10] studied the existence of CTGs in a spacetime with two spinning particles each one with magnetic moment equal