Table 1
Properties of the stellar sample.
Name | Sp. type | Ref. | [Fe/H] | N obs | Δt | ⟨ V ⟩ | σ | σ / ϵ | SB/ORB |
(d) | (km s-1) | (km s-1) | |||||||
|
|||||||||
HD 26 | CH | 10 | –1.3 | 110 | 11999 | –213.14 | 1.36 | 25 | ORB: |
HD 76396 | CH | 6 | – | 68 | 13217 | –61.73 | 1.67 | 30 | ORB+jitter? |
HD 145777 | CH | 3 | – | 32 | 2215 | 18.43 | 0.83 | 15 | SB |
HD 187216 | CH | 8 | –2.5 | 41 | 12373 | –115.08 | 4.49 | 82 | SB |
HIP 53522 | CH(-like) | 6, 9, 11 | –0.5 | 57 | 1816 | 32.49 | 5.54 | 100 | ORB |
HIP 53832 | CH(-like) | 6, 7, 11 | –0.8 | 38 | 1151 | –2.28 | 7.36 | 134 | ORB |
HE 0017+0055 | CEMP-rs | 1, 5, 12 | –2.4 | 25 | 1581 | –79.84 | 0.52 | 9.5 | SB+jitter? |
HE 0111-1346 | CEMP-s | 1, 5 | –1.9 | 52 | 1542 | 44.71 | 6.45 | 117 | ORB |
HE 0457-1805 | CEMP-s | 1, 5 | –1.5 | 29 | 1894 | 66.76 | 4.24 | 77 | ORB |
HE 0507-1653 | CEMP-s | 2, 5 | –1.8 | 30 | 1495 | 348.41 | 4.90 | 89 | ORB |
HE 1120-2122 | CEMP-s | 4 | – | 40 | 1948 | 108.6 | 3.79 | 69 | ORB+jitter? |
HE 1429-0551 | CEMP-s | 1, 2 | –2.5 | 39 | 1930 | –44.51 | 0.19 | 3.4 | SB? |
HE 2144-1832 | CEMP-s | 1 | – | 22 | 2170 | 141.79 | 0.60 | 11 | SB |
Notes. Nobs is the number of radial-velocity observations (including older measurements from McClure & Woodsworth 1990), Δt is their time span, ⟨ V ⟩ is the average velocity and σ its standard deviation, σ/ϵ is the ratio between the standard deviation and measurement error (estimated to be 55 m s-1). In column SB/ORB, the systems with close to 1 yr variations superimposed on the long-term orbit are flagged with the label “jitter?”.
Reference. (1) Goswami (2005); (2) Masseron et al. (2010); (3) Bidelman (1956); (4) Goswami et al. (2010); (5) Kennedy et al. (2011); (6) Hartwick & Cowley (1985); (7) Zamora et al. (2009); (8) Kipper & Jorgensen (1994); (9) this work; (10) Van Eck et al. (2003); (11) Sperauskas et al. (2015); (12) Jorissen et al. (2016).
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