1999MNRAS.310.1119K

We present extensive photometry and spectroscopy of the extremely hydrogen-deficient star, LSS 3184, recently discovered to be a rapid variable (period ∼0.1066d) strikingly similar to V652 Her. Over 95h of photometry confirms the reported variability, which is of rather low amplitude (ΔV∼0.03mag), defines the light curve with greater precision and establishes a much more accurate ephemeris (period ∼0.1065784d) to form a basis for detecting period change. Attention is drawn to the usefulness of a period-finding technique that fits harmonic components to the photometric observations. Spectroscopy shows a peak-to-peak variation in radial velocity of about 30kms^–1, which, when combined with the photometric observations, confirms the pulsational nature of the variability and strongly indicates that the pulsations are radial in nature.