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Radial and nonradial periods and growth rates of an AI Velorum model
Authors:J A Guzik
Institution:(1) Applied Theoretical Physics Division, Los Alamos National Laboratory, USA
Abstract:Walraven, Walraven and Balona recently discovered several new periodicities in addition to the well-known fundamental and first overtone periods of the high-amplitudedelta Scuti star AI Velorum. Linear nonadiabatic pulsation calculations were performed for an AI Velorum model of mass 1.96M odot, 24.05L odot, andT eff 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.
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