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Table 4.
Orbital properties of Aa, Ba, and Bb derived from the disengangled residual spectra, analogous to Table 4 from Hełminiak et al. (2017).
| Aa (SB1) | Ba+Bb (SB2) | Units | |
|---|---|---|---|
| P | 94.07 ± 0.11 | 8.653290 ± 0.000075 | Days |
| Tperi | 56024.1 ± 6.7 | 56050.3728 ± 0.0065 | Days |
| K1 | 22.11 ± 0.36 | 67.86 ± 0.26 | km s−1 |
| K2 | – | 68.26 ± 0.18 | km s−1 |
| γ | −26.34 ± 0.36 | −23.203 ± 0.082 | km s−1 |
| e | 0.037 ± 0.016 | 0.3713 ± 0.0017 | – |
| ω1 | 289 ± 26 | 13.14 ± 0.31 | ° |
| f(m) | 0.1052 ± 0.0051 | – | M⊙ |
| M1sin3i | – | 0.9076 ± 0.0056 | M⊙ |
| M2sin3i | – | 0.9023 ± 0.0070 | M⊙ |
| a1 sin i | 28.59 ± 0.51 | 7.497 ± 0.027 | 106 km |
| a2 sin i | – | 7.541 ± 0.018 | 106 km |
| σ1 | 1.545 | 1.05 | km s−1 |
| σ2 | – | 0.68 | km s−1 |
Notes. The values are consistent with Table 3 within the uncertainties.
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