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Radial Pulsations In 63 Herculis

Published online by Cambridge University Press:  12 April 2016

Bülent Uyaniker
Bülent Uyaniker*
Affiliation:
Physics Department, Middle East Technical University06531 Ankara, Turkey.

Abstract

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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
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 736 - 738
Copyright
Copyright © Astronomical Society of the Pacific 1993

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