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Resonance Effect of Binary Orbital Motion upon δ Scuti Type Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
The colour behaviour of θ Tucanae with orbital phase is shown. A break in the residuals is checked as the criterion for stopping the period search. A resonance of the dominant pulsational mode and the period of ellipticity is reported, with a Resonance number of 72.
- Type
- Part 1.2. Pulsations in Close Binaries
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- Copyright © Astronomical Society of the Pacific 2002