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Table 1
Combinations of fundamental stellar parameters covered by the model grid.
| T⋆ | log L⋆ | P | M⋆ | log (C–O) + 12 |
| [K] | [L⊙] | [d] | [M⊙] | [dex] |
|
|
||||
| 2600 | 3.70 | 294 | 0.75, 1.0 | 8.2, 8.5, 8.8 |
| 3.85 | 390 | 0.75, 1.0, 1.5, 2.0 | 8.2, 8.5, 8.8 | |
| 4.00 | 525 | 1.0, 1.5, 2.0 | 8.2, 8.5, 8.8 | |
|
|
||||
| 2800 | 3.55 | 221 | 0.75 | 8.2, 8.5, 8.8 |
| 3.70 | 294 | 0.75, 1.0 | 8.2, 8.5, 8.8 | |
| 3.85 | 390 | 0.75, 1.0, 1.5, 2.0 | 8.2, 8.5, 8.8 | |
| 4.00 | 525 | 1.0, 1.5, 2.0 | 8.2, 8.5, 8.8 | |
|
|
||||
| 3000 | 3.55 | 221 | 0.75 | 8.2, 8.5, 8.8 |
| 3.70 | 294 | 0.75, 1.0 | 8.2, 8.5, 8.8 | |
| 3.85 | 390 | 0.75, 1.0, 1.5, 2.0 | 8.2, 8.5, 8.8 | |
| 4.00 | 525 | 1.5 | 8.2, 8.5, 8.8 | |
|
|
||||
| 3200 | 3.55 | 221 | 0.75 | 8.2, 8.5, 8.8 |
| 3.70 | 294 | 0.75, 1.0 | 8.2, 8.5, 8.8 | |
Notes. The period is not an independent parameter but coupled to the stellar luminosity, see text. For each set of parameters listed here we varied the velocity and luminosity amplitude (Δup, fL) of the inner boundary.
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