Table 5.
Stellar mass (in solar units), surface gravity, envelope mass, and the surface chemical abundances by mass for the evolutionary sequences considered in this work.
| M⋆/M⊙ | log g (cgs) | log(Menv/M⋆) | X4He | X12C | X16O |
|---|---|---|---|---|---|
| 0.530 | 6.120 | −1.18 | 0.33 | 0.39 | 0.17 |
| 0.542 | 5.944 | −1.22 | 0.28 | 0.41 | 0.21 |
| 0.565 | 5.853 | −1.34 | 0.39 | 0.27 | 0.22 |
| 0.589 | 5.780 | −1.40 | 0.31 | 0.38 | 0.23 |
| 0.609 | 5.677 | −1.51 | 0.50 | 0.35 | 0.10 |
| 0.664 | 5.541 | −1.86 | 0.47 | 0.33 | 0.13 |
| 0.741 | 5.417 | −2.00 | 0.48 | 0.34 | 0.14 |
Notes. The values correspond to models with log(Teff) = 5.1 K at the stages before the evolutionary knee, that is, the maximum effective temperature possible (see Fig. 5).
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