  We obtain charged spherically symmetric black holes in the two-component
scalar Einstein-Maxwell-Friedberg-Lee-Sirlin model with a symmetry breaking
potential. These asymptotically flat black holes carry resonant scalar Q-hair.
As expected, these hairy black holes give rise to non-uniqueness. When
comparing these solutions with the corresponding charged boson stars and
Reissner-Nordstr\"om black holes, we find a different pattern in the case of a
massive real scalar component and a massless one. We demonstrate that, as the
real component becomes massless, the resonant hairy black holes bifurcate from
Reissner-Nordstr\"om black holes for sufficiently small gravitational coupling.
