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A survey of RR Lyrae models

Published online by Cambridge University Press:  15 February 2018

G. Bono  and
R.F. Stellingwerf
G. Bono
Affiliation:
Trieste Astronomical Observatory, Italy
R.F. Stellingwerf
Affiliation:
Los Alamos National Laboratory, NM

Abstract

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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).

Type
Theoretical Breakthroughs
Information
International Astronomical Union Colloquium , Volume 139: New Perspectives on Stellar Pulsation and Pulsating Variable Stars , 1993 , pp. 262
Copyright
Copyright © Cambridge University Press 1993