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Table 4

Complete set of (P,e) values currently available for CEMP-(r)s, CH and CH-like stars, along with the mass functions f(M1,M2) analysed in Sect. 5.1.

Name P e d/g f(M1,M2) [Fe/H] [i/Fe] (Ni(s) − Ni(scaled−solar)) N neut Ref.
× (Ai − 56) × 10-4
(d) (M⊙) Sr Zr La Pb Sr Zr La Pb
HE 0024-2523 3.41 0. d 0.050 –2.7 0.34 – 1.8 3.3 60 – 159 69443 6.97 1
HE 1046-1352 20.2 0. ? 0.057 –3.7 19
CS 29509-027 194 0.15 d 0.001 –2.0 2
G77-61 245.5 0. d – –4.0 3, 9
HE 1523-1155 309.3 0.27 g 0.004 –2.2 19, 20
HIP 53832 322.8 0.05 g 0.056 –0.8 4, 10
BD + 42°2173 328.3 0. g 0.005 – 5
CS 29497-030 342 0. d 0.002 –2.2 1.15 – 1.91 3.75 2308 – 714 678838 68.19 2, 18
HE 0151-0341 359.1 0. g 0.067 –2.5 11, 19
HIP 53522 361.1 0.36 g 0.070 –0.5 4
HE 0854+0151 389.9 0. ? 0.086 –1.8 19
HE 0111-1346 402.7 0.02 g 0.083 –1.9 4, 11
HE 0507-1653 405.0 0.00 g 0.015 –1.8 4, 11
HD 209621 407.4 0. g 0.074 –1.9 1.0 1.80 2.4 1.9 2880 9875 4049 17232 3.12 5, 12
CS 22948-27 426 0.02 g (rs) 0.033 –2.5 6, 13
BD + 02°3336 445.9 0.03 g 0.054 –0.5 7, 10
HE 0507-1430 447.0 0.01 g 0.060 –2.4 19, 21
HIP 99725 541.1 0.04 g 0.015 –0.1 22
BD + 08°2654a 571.1 0.0 g 0.044 – 5
HIP 2529 725. 0.0 g 0.001 – 22
HE 0002-1037 740.9 0.14 ? 0.064 –3.8 19
HD 5223 755.2 0.0 g 0.081 –2.1 5, 14
HIP 43042 1042 0.35 g 0.035 –0.5 22
HD 224959 1273 0.18 g 0.092 –2.1 5, 15
CS 22956-028 1290 0.22 d 0.076 –2.1 2
HD 198269 1295 0.09 g 0.107 –2.2 – 0.4 1.6 2.4 – 121 315 27549 2.80 5, 16
HD 202851 1295 0.06 g 0.083 –0.7 22
HE 0430-1609 1382 0.43 ? 0.002 –3.0 19
HD 201626 1465 0.10 g 0.022 –2.1 – 0.9 1.9 2.6 – 697 801 55049 5.65 5, 16
HE 2312-0758 1890 0.26 ? 0.014 –3.5 19
HE 1120-2122 2080 0.15 g 0.060 – 4
HIP 80769 2129 0.19 g 0.089 – 22
HE 0457-1805 2723 0.19 g 0.078 –1.5 4, 11
CS 22942-019 2800 0.10 g 0.036 –2.7 8, 17
HD 85066 2902 0.21 g 0.113 – 7
HD 30443 2954 0.0 g 0.024 – 5
HE 0319-0215 3078 0. ? 0.025 –2.3 19
CS 29497-034 4130 0.02 g (rs) 0.060 –2.9 6
HD 76396 13611 0.41 g 0.070 – 4, 5
HD 26 19634 0.08 g 0.075 –1.3 – 0.9 2.3 2.0 – 4396 12791 86592 10.38 4, 16

Notes. The column labeled “d/g” specifies whether the star is a dwarf or a giant. In that column, “rs” designates a CEMP-rs star. The stars are ordered according to increasing orbital periods. The quantities Ni and Nneut are defined in relation with Eq. (1).

Reference. (1) Lucatello et al. (2003); (2) Sneden et al. (2003b); (3) Dearborn et al. (1986); (4) this work; (5) McClure & Woodsworth (1990); (6) Barbuy et al. (2005); (7) McClure (1997); (8) Preston & Sneden (2001); (9) Plez & Cohen (2005); (10) Zamora et al. (2009); (11) Kennedy et al. (2011); (12) Goswami & Aoki (2010); (13) Allen et al. (2012); (14) Goswami et al. (2006); (15) Masseron et al. (2010); (16) Van Eck et al. (2003); (17) Preston & Sneden (2000); (18) Sivarani et al. (2004); (19) Hansen et al. (2016); (20) Aoki et al. (2007); (21) Beers et al. (2007); (22) Sperauskas et al. (2015).

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