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Spherical Oscillation Patterns

Published online by Cambridge University Press:  12 April 2016

W. Dean Pesnell
Affiliation:
Department of Physics, University of Florida, Gainesville, FL 32611USA
James M. Coggins
Affiliation:
Department of Computer Sciences, Michigan State University, East Lansing, MI 48825USA

Abstract

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Spherical harmonics are an integral part of the study of stellar pulsations. To gain an understanding of how the star is affected by non-radial pulsations, the radial part of the oscillation is plotted, with an assumed sinusoidal time variation. The amplitude of the motion is arbitrarily set at 20% of the radius.

Type
VI. Red Variables
Copyright
Copyright © Reidel 1980

References

Morse, P. M. and Feshbach, H.: 1953, Method of Theoretical Physics, McGraw - Hill Book Co., Inc. N. Y. Vol II, Ch. 10.Google Scholar
Jahnke, E. and Emde, F.: 1945, Table of Functions, Dover Publ., Inc. N. Y. Ch.7.Google Scholar
Disspla Pocket Manual: 1978, copyright 1975, Integrated Software Systems Corporation, San Diego, CA Google Scholar