Numerical modelling of the RR Lyrae instability strip

Details Numerical modelling of the RR Lyrae instability strip Numerical modelling of the RR Lyrae instability strip

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004coast.145...21s&link_type=abstract

Communications in Asteroseismology, vol. 145, p. 21-23

Physics

Scientific paper

Selected results are presented of an extensive model survey of the radial pulsation of HB stars using a turbulent convective (TC) code. The main goal of the investigation was to systematically map the possible pulsational modes in the classical instability strip. This contribution focuses on (i) the slope of the fundamental mode blue edge and (ii) double-mode RR Lyrae stars. The importance of the interplay between mode-selection effects and stellar evolution is emphasized in both cases.

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