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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. 11.

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﹩ for two representative models taken from the ﹩M=0.4758+0.0002﹩ M sequence and artificially modified by imposing a value ﹩B=0﹩ in the C‐O/He composition transition zone. Note that the scale is the same as in Fig. 9.

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