Modelling of RR Lyrae instability strips

Details Modelling of RR Lyrae instability strips Modelling of RR Lyrae instability strips

Feb 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001padeu..11..101s&link_type=abstract

Publications of the Astronomy Department of the Eötvös University No. 11, Proceedings of the National Postgraduate Reunion in As

Astronomy and Astrophysics

Astrophysics

Variable Stars, Rr Lyrae, Evolution, Turbulent Convection

Scientific paper

Recent studies indicates that the slope of the empirical blue edge of the RR Lyrae fundamental mode instability strip is irreconcilable with the theoretical blue edges. Nonlinear hydrodynamical pulsational code involving turbulent convection was used to follow fundamental/first overtone mode selection mechanism. This method combined with the results of horizontal branch evolutionary computations was applied to rethink the problem.

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