  In this work we calculate the angular deflection of light in the strong field
limit in two spacetimes which were previously studied within the
Eddington-inspired Born-Infeld gravity (EiBI), namely, a black hole and a
wormhole, both with topological charge. We show that the presence of the
parameters characterizing EiBI and the topological charge promote significant
changes in the angular deflection of light with respect to that one obtained in
Schwarzschild spacetime. Using the expression for angular deflection in the
strong field limit, we calculate the position and magnification of the
respective relativistic images.
