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Adiabatic Survey of Subdwarf B Star Oscillations. III. Effects of Extreme Horizontal Branch Stellar Evolution on Pulsation Modes

  • Authors: S. Charpinet, G. Fontaine, P. Brassard, and Ben Dorman

Charpinet et al. 2002 The Astrophysical Journal Supplement Series 140 469.

  • Provider: AAS Journals

Caption: Fig. 9.

Spectra of the relative rate of period change ﹩\dot{P_{k}}/ P_{k}﹩ as a function of the reduced period ﹩P_{k}[ l( l+1) ] ^{1/ 2}﹩ for g‐modes with ﹩k=1{\mbox{--}} 30﹩ and ﹩\ell =1{\mbox{--}} 3﹩. Each ensemble of two panels refers to a given evolutionary sequence. The upper (lower) panel corresponds to a representative model belonging to the first (second) phase of EHB evolution. The model number is indicated in the upper right‐hand corner of each panel.

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