Intensive photometry of southern Wolf-Rayet stars

We present results of an intensive photometric campaign on 17 of the brightest southern Wolf–Rayet stars. We report the detection of multi-periodicity in two stars: HD 50896 and HD 96548. It is likely that these periodicities are not coherent but are manifestations of the quasi-periodic variations seen in a few WR stars. A good example of these variations is given by HD 86161. A new eclipsing binary, HD 92740 has been discovered; other stars show periodic variations which can be explained by phase-dependent scattering of the secondary light as it traverses the Wolf–Rayet wind. An important conclusion of this study is that not a single example was found of short-period variations which can be attributed to pulsation.