| Abstract
| - We report on the identification of the optical counterpart of the binary millisecond pulsar PSR J1911-5958A, located in the outskirts of the globular cluster NGC 6752. At the position of the pulsar we find an object with $V=22.08$, $B-V=0.38$, $U-B=-0.49$. The object is blue with respect to the cluster main sequence by 0.8 mag in $B-V$. We argue that the object is the white dwarf companion of the pulsar. Comparison with white dwarf cooling models shows that this magnitude and colors are consistent with a low-mass white dwarf at the distance of NGC 6752. If associated with NGC 6752, the white dwarf is relatively young, $\la$$2\,$Gyr, which sets constraints on the formation of the binary and its ejection from the core of the globular cluster.
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