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Table B.8

Fitted Keplerian and drift parameters for triple systems.

Parameters HD 71827 HD 212735 BD+212816
Pb (day) 15.052366 ± 0.000051 37.940879 ± 0.000092 788.91 ± 0.10
Kb (m s−1) 2173.9 ± 1.5 5406.4 ± 1.8 3137 ± 11
eb 0.07645 ± 0.00068 0.18327 ± 0.00037 0.2275 ± 0.0052
ωb (°) 57.02 ± 0.42 101.80 ± 0.22 70.98 ± 0.74
T0,b–2.4 106 (day) 57 424.287 ± 0.017 57 585.784 ± 0.020 56 852.8 ± 1.1

Linear drift (m s−1 yr−1) −438.984 ± 0.027 −90.12 ± 0.11 15 ± 14
Quad drift (m s−1 yr−2) −40.80921 ± 0.00033
Cubic drift (m s−1 yr−2) −1.5666752 ± 0.0000031
Pc (day) >7000 >7000 >8000

γS+ (km s−1) −36.9407 ± 0.0020 −24.8571 ± 0.0028 −32.141 ± 0.017
σOC,S+ (m s−1) 6.22 1.50 5.13
γS (km s−1) fixed fixed
σOC,S (m s−1) 5.75 10.6

f(Mb) (10−6 M) 15.881 ± 0.033 590.18 ± 0.59 2329 ± 32
Mb sini (MJ) 27.43 ± 0.89 92.5 ± 3.0 120.4 ± 4.2
ab (AU) 0.1228 ± 0.0020 0.2328 ± 0.0037 1.627 ± 0.027
f(Mc) (10−6 M) 3805 ± 351 77.9 ± 3.7 1.9 ± 5.4
Mc sini (MJ) >163 >45 >5
aci (AU) >7.5 >7.3 >7.2

Notes. The minimum possible period for the third object is given with the corresponding m sin i and semi-major axis derived when fixing the period at this value. In both cases, the orbit of component 1 was derived assuming the drift. In all cases, we fixed the SOPHIE (or Elodie) and SOPHIE+ relative RV offset to 0 m s−1.

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