Table A.2
Derived physical properties of the WASP-11/HAT-P-10 system based on the prediction of different theoretical models.
| Claret models | Y2 models | BaSTI models | VRSS models | DSEP models | ||
|
|
||||||
| Kb ( km s-1) | 129.9 ± 3.2 | 127.7 ± 2.0 | 127.5 ± 1.9 | 127.5 ± 2.3 | 128.4 ± 2.1 | |
| M⋆ ( M⊙) | 0.846 ± 0.063 | 0.804 ± 0.039 | 0.800 ± 0.036 | 0.800 ± 0.043 | 0.818 ± 0.038 | |
| R⋆ (R⊙) | 0.785 ± 0.023 | 0.772 ± 0.013 | 0.771 ± 0.015 | 0.771 ± 0.014 | 0.777 ± 0.012 | |
| log g⋆ (cgs) | 4.576 ± 0.016 | 4.569 ± 0.016 | 4.568 ± 0.015 | 4.568 ± 0.018 | 4.571 ± 0.018 | |
| Mp (MJup) | 0.508 ± 0.028 | 0.492 ± 0.020 | 0.490 ± 0.019 | 0.490 ± 0.024 | 0.497 ± 0.023 | |
| Rp (RJup) | 1.006 ± 0.031 | 0.989 ± 0.019 | 0.987 ± 0.020 | 0.987 ± 0.023 | 0.995 ± 0.022 | |
| ρp (ρJup) | 0.467 ± 0.028 | 0.475 ± 0.025 | 0.476 ± 0.026 | 0.476 ± 0.027 | 0.472 ± 0.026 | |
| Θ | 0.0531 ± 0.0021 | 0.0540 ± 0.0016 | 0.0541 ± 0.0017 | 0.0541 ± 0.0019 | 0.0537 ± 0.0019 | |
| a (AU) | 0.04447 ± 0.00111 | 0.04373 ± 0.00069 | 0.04365 ± 0.00065 | 0.04365 ± 0.00080 | 0.04398 ± 0.00070 | |
| Age (Gyr) |
|
|
... | ... |
|
|
Notes. In each case gp = 12.45 ± 0.50 m s-2, ρ⋆ = 1.748 ± 0.074ρ⊙ and Teq = 992 ± 14 K. We were not able to constrain a reasonable value for the age of the WASP-11/HAT-P-10 system by using the BaSTI and VRSS models, because the evolution of a star of the mass of WASP-11 is short for times shorter than the age of the Galaxy.
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