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Table A.3

Same as Table A.1 for S (and C) stars.

Name (HD/DM) Period (d) e f(M) (M) Ref.

Extrinsic S stars
121447 185.7 ± 0.1 0.01 ± 0.01 0.025 ± 0.001 1
95875 197.2 ± 0.3 0.0 0.061 ± 0.007 19 (Hen4-108)
–25°10393 346.6 ± 0.03 0.104 ± 0.003 0.066 ± 0.001 0, 19 (Hen 4-147)
191589 377.3 ± 0.1 0.250 ± 0.003 0.394 ± 0.005 4
189581 614 ± 1 0.39 ± 0.02 (1.3 ± 0.1) × 10-5 0
22649 596.2 ± 0.2 0.09 ± 0.02 0.037 ± 0.003 15
35155 638.2 ± 0.3 0.07 ± 0.03 0.032 ± 0.003 16 (V1261 Ori)
332077 669.1 ± 1.0 0.077 ± 0.007 1.25 ± 0.02 10
+24°620 773.4 ± 5.5 0.06 ± 0.03 0.042 ± 0.005 10
+22°700 849.5 ± 8.8 0.08 ± 0.06 0.043 ± 0.008 10
+23°3093 1008.1 ± 4.8 0.39 ± 0.03 0.045 ± 0.005 10
215336 1143.3 ± 0.6 0.021 ± 0.003 0.039 ± 0.003 0
9810 1147 ± 2 0.21 ± 0.01 0.019 ± 0.001 19 (Hen 4-2)
63733 1160.7 ± 8.9 0.23 ± 0.03 0.025 ± 0.003 4
191226 1210.4 ± 4.3 0.19 ± 0.02 0.013 ± 0.001 17
+28°4592 1252.9 ± 3.5 0.09 ± 0.02 0.016 ± 0.001 4
246818 2548.5 ± 73.2 0.18 ± 0.11 0.004 ± 0.002 4
49368 2996 ± 67 0.36 ± 0.05 0.022 ± 0.003 4
+23°3992 3096 ± 42 0.10 ± 0.03 0.034 ± 0.004 4
343486 3166 ± 38 0.24 ± 0.03 0.039 ± 0.005 4
+21°255(S) 4137 ± 317 0.21 ± 0.04 0.032 ± 0.004 4
170970 4651 ± 10 0.19 ± 0.01 0.0213 ± 0.0007 0
+31°4391 6757 ± 37 0.14 ± 0.03 0.03 ± 0.01 0
+79°156 11119 ± 69 0.44 ± 0.01 0.022 ± 0.002 0
184185 17490: 0.37: 0
288833 17565: 0.42: 0
218634 90359: 0.55: 0
Symbiotic S and C stars
–28°3719 399.1 ± 0.1 <0.002 0.020 ± 0.001 0 (Hen 4-18)
V420 Hya 750.0 ± 0.2 0.092 ± 0.002 0.0928 ± 0.0004 0, 19 (Hen 4-121)
59643 1305 ± 4 0.18 ± 0.03 0.027 ± 0.003 18 (C)
ER Del 2056 ± 2 0.233 ± 0.004 0.069 ± 0.001 16
7351 4559 ± 9 0.11 ± 0.01 0.062 ± 0.001 0

Reference. (To Tables A.1A.3:) (0) Jorissen et al. (in prep.); (1) Jorissen et al. (1995); (2) Griffin (2008); (3) Stefanik et al. (2011); (4) Udry et al. (1998a); (5) Udry et al. (1998b); (6) McClure & Woodsworth (1990); (7) Mermilliod et al. (2007); (8) Griffin & Griffin (1980); (9) Griffin et al. (1996); (10) Jorissen et al. (1998); (11) Griffin (2006); (12) Griffin (1991); (13) Griffin & Keenan (1992); (14) Griffin (2009); (15) Griffin (1984); (16) Boffin et al. (2014); (17) Carquillat et al. (1998); (18) Carquillat & Prieur (2008); (19) Van Eck et al. (2000); (20) Fekel (priv. comm.); (21) a new orbital solution has been computed from McClure & Woodsworth (1990) data, and the non-zero eccentricity has been adopted from that new computation (despite being compatible with a circular orbit); (22) a solution with P = 10 480 d, e = 0.36, and f(M) = 0.11 ± 0.01M is also possible, although less probable given the large value of the mass function.

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