Discovery of additional pulsation modes in AI Velorum

Astronomy and Astrophysics – Astronomy

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Cepheid Variables, Dwarf Stars, Periodic Variations, Stellar Oscillations, Astronomical Photometry, Scutum Constellation, Vibration Mode

Scientific paper

Consideration is given to the analysis of 13 394 blue-light photometric observations of the high-amplitude Delta Scuti star AI Velorum. These data were obtained for six seasons spanning 38 years. It is found that in addition to the well-known fundamental and first-overtone radial modes, two previously undiscovered periodicities are present; one of them was initially suspected by Walraven many years ago. These periodicities are present in every season. A tentative identification in terms of the third and fifth radial overtones is proposed. A nonlinear interaction term between one of the new periodicities and the first overtone is present. A fifth mode, intermediate in period between the fundamental and first overtone may also be present. It is also found that the period of the first overtone is increasing at a steady rate, but that there is little or no change in the period of the fundamental mode over an interval of more than 50 years.

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