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Table 1.
Period P, eccentricity e, metallicity [Fe/H], mass M, and corresponding references, for five Ba, CH, or S giants with outlying orbital properties according to Fig. 9.
| ID 1 | ID 2 | Type | P [days] | e | Orbit ref. | [Fe/H] | M [M⊙] | M ref. |
|---|---|---|---|---|---|---|---|---|
| HD 24035 | HIP 17402 | Ba | 377.8 ± 0.3 | 0.02 ± 0.01 | Udry et al. (1998a) | -0.23 | 1.3 ± 0.3 | Jorissen et al. (2019) |
| BD+41°2150 | HIP 53832 | CH | 322.84 ± 0.08 | 0.055 ± 0.001 | Jorissen et al. (2016) | -0.8 | 1.27 ± 0.2 | This work(1) |
| HD 123949 | HIP 69290 | Ba | 8523 ± 8 | 0.9162 ± 0.0003 | Jorissen et al. (2019) | -0.23 | 1.3 ± 0.3 | Jorissen et al. (2019) |
| HD 134698 | BD-09°4082 | Ba | ∼10005 | ∼0.95 | Jorissen et al. (2019) | -0.57 | 1.5 ± 0.2 | Jorissen et al. (2019) |
| HD 191589 | HIP 99312 | S | 377.3 ± 0.1 | 0.250 ± 0.003 | Udry et al. (1998a) | -0.3 | 1.0 | Shetye et al. (2018) |
Notes. Their location on the HR diagram is shown in Fig. 10.
(1)
Following the method used by Jorissen et al. (2019) and Escorza et al. (2019a).
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