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Nonlinear RR Lyrae Models with New Livermore Opacities

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Abstract

A. N. Cox recently showed that a 20% opacity decrease in the 20,000–30.000 K region as indicated by the new Livermore OPAL opacities reconciles the discrepancy between pulsation and evolution masses of double-mode RR Lyrae variables. Nonlinear hydrodynamic calculations were performed for RR Lyrae models of mass 0.75M , 51L , and Z = 0.0001 (Osterhoff II type) including this opacity decrease. The Stellingwerf periodic relaxation method was used to converge the models to a limit cycle, and the Floquet matrix eigenvalues calculated to search for a tendency of the fundamental mode to grow from the full-amplitude overtone solution, and the overtone mode to grow from the full-amplitude fundamental solution, thereby predicting double-mode behavior. Models of T eff < 7000 K with the opacity decrease have positive fundamental-mode growth rates in the overtone solution, in contrast to earlier results by Hodson and Cox (1982), and models with T eff > 7000 have positive 1st overtone growth rates in the fundamental-mode solution, but double-mode behavior was not found.

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© 1993 Springer Science+Business Media Dordrecht

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Guzik, J.A., Cox, A.N. (1993). Nonlinear RR Lyrae Models with New Livermore Opacities. In: Takeuti, M., Buchler, JR. (eds) Nonlinear Phenomena in Stellar Variability. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1062-4_46

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  • DOI: https://doi.org/10.1007/978-94-011-1062-4_46

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-4462-2

  • Online ISBN: 978-94-011-1062-4

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