 |
| Figure 1: Comparison of the scaled solar evolutionary tracks for our standard solar model (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. |
|
|
| Figure 1: Comparison of the scaled solar evolutionary tracks for our standard solar model (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. |