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A survey of RR Lyrae models
Published online by Cambridge University Press: 15 February 2018
Abstract
An extensive grid of non-linear pulsating models of RR Lyrae stars have been computed. To simulate the outer regions of these variables a non-local and time-dependent treatment of convective transport has been adopted. In this poster we briefly describe some new features of the instability strip (IS).
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- Copyright © Cambridge University Press 1993