Optical variability of the B-type star HD 105382: Pulsation or rotation?

We present ground-based multi-colour Geneva photometry and high-resolution high S/N spectra of the variable B-type star HD 105382. We provide evidence that this star is not a Be star, as indicated in the literature. The monop eriodic variability found in the Hipparcos data is confirmed in our ground- based follow-up observations. All existing data give rise to the detection of the period of 1.295 days. We try to interpret the variability of the sta r in terms of a non-radial g-mode pulsation model and of a rotational modul ation model. None of these two is able to explain the observed line-profile variations in full detail.