  The detection of the orbital period of 4.36his reported for the new
Intermediate Polar 1 WGA 1958.2+3232. The orbital period was derived from
time-resolved photometric and spectral observations. We also confirmed the 733
sec spin period of the White Dwarf consistent with the X-ray pulsations and
were able to distinguish the beat period in the light curve. Strong modulations
with orbital period are detected in the emission spectral lines from spectral
observations. They show the presence of a bright hot spot on the edge of the
accretion disk.
  The parameters of this recently discovered Intermediate Polar are determined.
