  Properties of the motion of electrically charged particles in the background
of the Gibbons-Maeda-Garfinkle-Horowitz-Strominger (GMGHS) black hole is
presented in this paper. Radial and angular motion are studied analytically for
different values of the fundamental parameter. Therefore, gravitational
Rutherford scattering and Keplerian orbits are analysed in detail. Finally,
this paper complements previous work by Fernando for null geodesics (Phys. Rev.
D 85: 024033, 2012), Olivares & Villanueva (Eur. Phys. J. C 73: 2659, 2013) and
Blaga (Automat. Comp. Appl. Math. 22, 41 (2013); Serb. Astron. J. 190, 41
(2015)) for time-like geodesics.
