  In this paper, charged black holes in general relativity coupled to
Born-Infeld electrodynamics are studied as gravitational lenses. The positions
and magnifications of the relativistic images are obtained using the strong
deflection limit, and the results are compared with those corresponding to a
Reissner-Nordstrom black hole with the same mass and charge. As numerical
examples, the model is applied to the supermassive Galactic center black hole
and to a small size black hole situated in the Galactic halo.
