In this paper we consider the drag force problem in the STU model. Already this problem and related topics were studied in N=4 SYM theory. Here we study the same problem in N=2 supergravity theory with an R-charge black hole (the STU model). This paper extends our previous work [1,2] by studying more general charge configurations and by taking into account the effect of a constant electromagnetic field and higher derivative corrections. We consider a single quark and a q q̅ pair in a three

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... e non-extremal black hole background. First by using the AdS/CFT correspondence, we obtain the drag force, the diffusion coefficient, the total energy and momentum, quasinormal modes, and the effect of higher derivative corrections for the single quark. Next we calculate the drag force for a q q̅ pair which rotates around its center of mass. For the first time we study the motion of a rotating q q̅ pair in N=2 supergravity theory. We show that our results in the near-extremal limit agree with the energy loss of the moving quark which was calculated in the N=4 SYM plasma.