  Time-resolved observations of a 6' x 6' field, containing the position error
boxes of the X-ray source 1WGA J1958.2+3232, were performed in June 1999 with
the 91 cm Catania telescope, equipped with a Photon Counting Intensified CCD.
The star recently proposed as the optical counterpart of the 1WGA J1958.2+3232,
exhibited a strong optical modulation with a period compatible with that seen
in X-ray (~12 min). The optical modulation was detected again in September and
October 1999. These results confirm the identification of the optical
counterpart and support the classification of 1WGA J1958.2+3232 as a
cataclysmic variable, possibly an Intermediate Polar. Modulation at period
twice as large was also found in one observation run, suggesting that the true
spin period of the White Dwarf could be 24 min rather than 12 min, thus 1WGA
J1958.2+3232 appears to be, among the IPs, the slowest rotator which exhibit
double peaked spin profile.
