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Radial Pulsations In 63 Herculis
Published online by Cambridge University Press: 12 April 2016
Abstract
Constructing a theoretical model of 1.88 M⊙ pulsation properties of 63 Her have been analyzed. For the model, In question, pulsation periods in the fundamental mode and first two overtones have been derived by solving the linearized pulsation equations. The model has been found to be vibrationally stable.
- Type
- VIII. Asteroseismology: observation
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- Copyright © Astronomical Society of the Pacific 1993