Table 2
Input parameters covered by the model grids.
| M* | T* | log L* ∕L⊙ | P | Δup | fL | log[C-O] |
|---|---|---|---|---|---|---|
| (M⊙) | (K) | (d) | (km s−1) | +12 (dex) | ||
| 1.0 | 2600 | 3.70 | 294 | 2, 4, 6 | 2 | 8.2, 8.5, 8.8 |
| 3.85 | 390 | 2, 4, 6 | 2 | 8.2, 8.5, 8.8 | ||
| 4.00 | 525 | 2, 4, 6 | 2 | 8.2, 8.5, 8.8 | ||
| 1.0 | 2800 | 3.70 | 294 | 2, 4, 6 | 2 | 8.2, 8.5, 8.8 |
| 3.85 | 390 | 2, 4, 6 | 2 | 8.2, 8.5, 8.8 | ||
| 4.00 | 525 | 2, 4, 6 | 2 | 8.2, 8.5, 8.8 | ||
| 1.0 | 3000 | 3.70 | 294 | 2, 4, 6 | 2 | 8.2, 8.5, 8.8 |
| 3.85 | 390 | 2, 4, 6 | 2 | 8.2, 8.5, 8.8 | ||
| 4.00 | 525 | 2, 4, 6 | 2 | 8.2, 8.5, 8.8 | ||
| 1.0 | 3200 | 3.70 | 294 | 2, 4, 6 | 2 | 8.2, 8.5, 8.8 |
| 3.85 | 390 | 2, 4, 6 | 2 | 8.2, 8.5, 8.8 | ||
| 4.00 | 525 | 2, 4, 6 | 2 | 8.2, 8.5, 8.8 | ||
Notes. The stellar parameters (mass, effective temperature and luminosity) are listed in Cols. 1–3. The pulsation parameters (period, piston velocity andscaling factor for the luminosity amplitude) describing the sinusoidal variations at the inner boundary are listed in Cols. 3–6. Lastly, the carbon excess is listed in Col. 7. Note that the period P is not an independentparameter, but coupled to the stellar luminosity by the period-luminosity relation in Feast et al. (1989).
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