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Table 18

Ap stars with magnetically resolved lines with a known orbital period (or a meaningful lower limit thereof).

HD/HDE P rot P orb e f(M) Ref.
(d) (d) (M)

2453 521 2850
9996 7962 227.81 0.512 0.0273
12288 34.9 1546.5 0.342 0.102
18078 1358 978 1
29578 1800 926.7 0.377 0.070
50169 2900 1764 0.47 0.0009
55719 3650 46.31803 0.1459 0.522
59435 1360 1386.1 0.285 a 2
61468 322 27.2728 0.1723 0.1309
65339 8.02681 2422.04 0.718 0.149 1
81009 33.984 10700 0.718 b 3
94660 2800 848.96 0.4476 0.331
116114 27.61 ~ 4000 1
116458 148.39 126.233 0.143 0.0357
137909 18.4868 3858.13 0.534 0.1955 4
142070 3.3718 2500 1
144897 48.57 2200
165474 3300 2200
187474 2345 689.68 0.4856 0.0646
200311 52.0084 1800
201601 35 400 100 200 0.56 c 5

Notes.

(a)

SB2: M1 sin3i = 2.809 M, M2 sin3i = 2.614 M.

(b)

Visual binary: M1 = 2.6 M, M2 = 1.6 M.

(c)

Visual binary.

Reference. (1) Carrier et al. (2002); (2) Wade et al. (1999); (3) Wade et al. (2000a); (4) North et al. (1998); (5) Stelzer et al. (2011).

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