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The Effect of a Close Binary upon Stellar Pulsation
Published online by Cambridge University Press: 12 April 2016
Abstract
Through tidal deformation of the equilibrium state, the p-mode oscillations may show apparently complicated features. I discuss the fundamental characteristics of the tidally forced oscillation, and show the possibility that it leads to a triplet fine structure in the frequency spectrum of p-modes.
- Type
- Part 1.2. Pulsations in Close Binaries
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- Copyright © Astronomical Society of the Pacific 2002