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| Figure 2: Comparison of the alpha-enhanced evolutionary tracks for Z=0.001, 1Mo models (from the pre-Main Sequence to the tip of the RGB) computed with the AF94 and F05 scaled solar opacities, and the appropriate solar mixing length calibrations. |
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| Figure 2: Comparison of the alpha-enhanced evolutionary tracks for Z=0.001, 1Mo models (from the pre-Main Sequence to the tip of the RGB) computed with the AF94 and F05 scaled solar opacities, and the appropriate solar mixing length calibrations. |