Physics
Scientific paper
Dec 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997mnras.292..621p&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 292, p. 621
Physics
16
Variable Stars, Stellar Oscillations, F Stars, Stellar Rotation, O Stars, Light Curve, Astronomical Photometry, Power Spectra, Stellar Physics
Scientific paper
We present multisite photometric observations of the F0 IV star HR 2740=QW Pup that reveal it to be a Gamma Dor type variable pulsating with four frequencies: 1.0434, 0.9951, 1.1088 and 0.9019/d. These data were obtained over a time baseline spanning from January 14 to February 11, 1997. The 1.0434/d 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. Physical parameters were also derived for all the well-known Gamma Dor stars, confirming that this class is very homogenous. In the framework of the campaign, two Ap stars were also observed. The photometric differences between these rotating variables and HR 2740 are emphasized, corroborating the pulsational nature of the Gamma Dor stars. It is further demonstrated that the rotational splitting cannot be a suitable explanation of the observed frequency content of HR 2740.
Alwis D. de
Breuer Felix
Haupt Hermann
Koen Chris
Martinez Pablo
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