  The most violent strange mode pulsations (SMPs) are expected in classical WR
stars, the bare, compact helium-burning cores of evolved massive stars, where
SMPs are predicted to manifest themselves in cyclic photometric variability
with periods ranging from minutes to hours and amplitudes in the several to
tens of mmag range. Since WR\,2 is one of the hottest WR stars known, it should
make it an excellent candidate for SMPs. However, our high-precision near
infrared photometric campaign shows no periodic variations with an amplitude
higher than 2.5 mmag on a timescale of ~6 hours, which is more than an order of
magnitude smaller than the theoretical predictions.
