Table 3.
Orbital properties of Aa, Ba, and Bb derived directly from the RV measurements, analogous to Table 4 from Hełminiak et al. (2017).
Aa (SB1) | Ba+Bb (SB2) | Units | |
---|---|---|---|
P | 94.10 ± 0.11 | 8.653243 ± 0.000073 | Days |
Tperi | 56027.4 ± 7.8 | 56050.3738 ± 0.0067 | Days |
K1 | 22.19 ± 0.34 | 67.72 ± 0.25 | km s−1 |
K2 | – | 68.09 ± 0.16 | km s−1 |
γ | −26.45 ± 0.25 | 23.203 ± 0.077 | km s−1 |
e | 0.032 ± 0.015 | 0.3701 ± 0.0015 | – |
ω1 | 302 ± 30 | 13.18 ± 0.31 | ° |
f(m) | 0.1063 ± 0.0049 | – | M⊙ |
M1sin3i | – | 0.9029 ± 0.0052 | M⊙ |
M2sin3i | – | 0.8980 ± 0.0066 | M⊙ |
a1 sin i | 28.69 ± 0.44 | 7.486 ± 0.026 | 106 km |
a2 sin i | – | 7.527 ± 0.017 | 106 km |
σ1 | 1.56 | 1.08 | km s−1 |
σ2 | – | 0.66 | km s−1 |
Notes. Tperi is measured relative to BJD = 2 400 000; that is, Tperi = BJD − 2 400 000. Compared to the previous analysis by Hełminiak et al. (2017), we obtain lower values of a sin i for all three components; other properties are similar.
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