Abstract

We present multi-site photometric observations of the F0 IV star HR 2740=QW Pup that reveal it to be a γ Dor type variable pulsating with four frequencies: 1.0434, 0.9951, 1.1088 and 0.9019 d-1. These data were obtained at the European Southern Observatory and the South African Astronomical Observatory over a time baseline spanning from 1997 January 14 to February 11. The 1.0434-d-1 term dominates in amplitude (10 mmag) over the other three (each less than 5 mmag); the light curve comprising these four frequencies seems to be very stable and no residual power is left in the power spectrum. During the analysis particular attention was paid to methodological aspects, which cannot be neglected considering the proximity of the frequencies to 1 d-1. Physical parameters were also derived for all the well-known γ Dor stars, confirming that this class is very homogenous. In the framework of the campaign, two Ap stars (OU Pup�HR 2746 and PR Pup�HR 2761) were also observed. The photometric differences between these rotating variables and HR 2740 are emphasized, corroborating the pulsational nature of the γ Dor stars. It is further demonstrated that the rotational splitting cannot be a suitable explanation of the observed frequency content of HR 2740. © 1997 RAS.