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An Extended Work Integral for Pulsating Stars

Published online by Cambridge University Press:  12 April 2016

Norman R. Simon
Norman R. Simon*
Affiliation:
Behlen Laboratory of Physics, University of Nebraska-Lincoln

Extract

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This paper contains a preliminary report on research aimed at extending the pulsational work integral to next highest order beyond the linear regime.

We begin by writing the integral in fully nonlinear form (Cox and Giuli 1968), normalized by the stellar luminosity L

Type
V. Cepheids of Populations I and II
Information
International Astronomical Union Colloquium , Volume 58: Stellar Hydrodynamics , August 1980 , pp. 437 - 442
Copyright
Copyright © Reidel 1980

References

Cox, J. P. and Giuli, R. T. 1968, Principles of Stellar Structure (New York: Gordon and Breach), Vol. 2.Google Scholar
Simon, N. R. 1980, Ap. J. 237, 175.Google Scholar
Simon, N. R., Cox, A. N. and Hodson, S. W. 1980, Ap. J. 237, 550.Google Scholar
Stellingwerf, R. F. 1975, Ap. J. 195, 441.Google Scholar