Table 1.
Estimates of νrot and P0 for the evolutionary model of a γ Dor star (Model A of Christophe et al. 2018).
| νrot [μHz] | νrot [d−1] | P0 [103 s] | a | fi/f0 |
||
|---|---|---|---|---|---|---|
| Kelvin | Rossby | |||||
| Rossby modes with m = −1 and k = −2 | ||||||
| It. 1 | 7.66 | 0.662 | 1.57 | |||
| It. 15 | 7.032(2) | 0.6076(2) | 4.47(1) | −0.99 | 1.01–1.47 | |
| Kelvin g-modes with m = 1 | ||||||
| It. 1 | 6.64 | 0.574 | 4.03 | |||
| It. 5 | 6.944(8) | 0.6000(7) | 4.49(1) | 0.99 | 1.002–1.036 | |
| Kelvin and Rossby modes | ||||||
| It. 1 | 6.91 | 0.597 | 4.31 | |||
| It. 6 | 7.015(2) | 0.6061(1) | 4.565(3) | 0.27 | 1.002–1.035 | 1.01–1.46 |
| True value | 7 | 0.605 | 4.579 | |||
Notes. The numbers in the parentheses indicate the formal uncertainties in the last digit of each estimate, which correspond to the 99% confidence intervals. Correlation coefficients a between the estimates of νrot and P0 are given in the fifth column. The range of fi/f0 is given for the converged value of νrot in the sixth and seventh column for Kelvin and Rossby modes, respectively. The results of Paper I are reproduced in the seventh and eighth row.
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