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. 1999 Sep 16;2(1):2. doi: 10.12942/lrr-1999-2

Figure 7.

Figure 7

The upper graph shows the numerically obtained f-mode frequencies plotted as functions of the mean stellar density. In the second graph the functional ω is plotted as a function of the compactness of the star (M and R are in km, ωf-mode and ωw-mode in kHz). The letters A, B, C, … correspond to different equations of state for which one can refer to [19].