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Table 3

Overview of the known multiplicity of the objects studied in this article.

HD SB1 SB2 Astrometric or visual

1909 X
7374 X 1
11753 X 1
14228 1
19400 1
21933 x  ⟨ 1 ⟩ 
23950 x
27295 X
27376 X 2+
28217 X
29589 x 1
31373 x
32964 X 1+
33647 X
33904  ⟨ 1 ⟩ 
34364 Xa
34880 X
35548 X b
36881 X
37752
38478
42657 x 1+
49606 X 1
51688 x 1
53244 x  ⟨ 1 ⟩ 
53929 x  ⟨ 1 ⟩ 
59067 3+
63975
65949 X
65950 X
66259 X  ⟨ 1 ⟩ 
66409 X 1
68099 x
68826 XXd
70235
71066 x 3
71833 1
72208 X  ⟨ 1 ⟩ 
73340
75333 X 1+e
78316 X
90264 X  ⟨ 1 ⟩ 
101189  ⟨ 1 ⟩ 
110073 X
120709 X
124740 X
129174 X 1+
141556 Xa
144661 x
144844 X 1
158704 X
165493 X
178065 X
216494 X
221507  ⟨ 1 ⟩ 
224926

41040 X X c

Notes. (a) There are hints for a third component in these systems. (b) The visible component is identical with the SB2 system. (c) The visible component is identical with the SB1 system. (d) HD 68826 consists of two SB2 systems. (e) In fact, we see the two visual components as one.

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