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Table C.1.
Toy model parameter values used in the simulation shown in Fig.C.1, based on the parameters values of V456 Cyg (Van Reeth et al. 2022b).
| Parameter | Value |
|---|---|
| orbital frequency νorb (d−1) | 1.122091 |
| inclination angle i (°) | 83.198 |
| stellar mass M1 (M⊙) | 1.859 |
| stellar mass M2 (M⊙) | 1.576 |
| stellar radius R1 (R⊙) | 1.588 |
| stellar radius R2 (R⊙) | 1.507 |
| linear LD coefficient μ1 | 0.248 |
| linear LD coefficient μ2 | 0.285 |
| light contribution L1 | 0.6 |
| light contribution L2 | 0.4 |
| third light L3 | 0.0 |
| pulsation frequency νpuls, in (d−1) | 1.9491 |
| pulsation amplitude A | 0.005 |
| amplitude distortion A′ | 0.667 |
| mode identification (k, m) | (0,1) |
Notes. The binary parameters are listed in the top half of the table, the asteroseismic ones in the bottom half.
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