Figure 1: SOLA coefficients c_{nl} as a function of mode turning point. Modes for l=1, 2, 3 and 4 are identified by crosses, asterisks, circles, and squares respectively. Coefficients for the higher values of l are indicated by points. | |
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Figure 2: Evolutionary tracks in a theoretical HR diagram for stellar models of . The tracks are plotted from ZAMS up to the ages indicated, roughly corresponding to the total main sequence life time. | |
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Figure 3: The scaled moment of inertia normalised to the solar value versus the mean stellar density in solar units, for the stellar models of Fig. 2. For all models the mean density and decrease as a function of time while on the main sequence. | |
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