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Radial and Nonradial Periods and Growth Rates of an AI Velorum Model

Published online by Cambridge University Press:  12 April 2016

J. A. Guzik
J. A. Guzik*
Affiliation:
Applied Theoretical Physics Division, Los Alamos National Laboratory

Abstract

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Walraven, Walraven and Balona recently discovered several new periodicities in addition to the well-known fundamental and first overtone periods of the high-amplitude δ Scuti star AI Velorum. Linear nonadiabatic pulsation calculations were performed for an AI Velorum model of mass 1.96M⊙, 24.05L⊙, and Teff 7566 K for the radial and low-degree nonradial modes to help verify the tentative identifications made by Walraven, et al. Comparison of the calculated periods with the observations suggests some alternatives to the identifications proposed by Walraven, et al.

Type
III. Models
Information
International Astronomical Union Colloquium , Volume 134: Nonlinear Phenomena in Stellar Variability , 1993 , pp. 321 - 323
Copyright
Copyright © Kluwer 1993

References

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