Table 3
Overview of the known multiplicity of the objects studied in this article.
HD | SB1 | Astrometric | Comment |
or visual | |||
|
|||
6532 | |||
9289 | 1 | ND | |
12932 | 1 | ND | |
19918 | |||
24712 | |||
42659 | |||
86181 | |||
99563 | 1 | CD | |
101065 | |||
116114 | X? | 1 | NR |
119027 | |||
122970 | |||
134214 | |||
137949 | |||
150562 | |||
154708 | 1 | ND | |
161459 | |||
166473 | |||
176232 | |||
185256 | |||
190290 | |||
193756 | |||
196470 | |||
201601 | 3 | CD+NR+NR | |
203932 | 1 | ND | |
213637 | |||
217522 | |||
218495 | |||
|
|||
Magnetic Ap stars | |||
|
|||
40711 | X? | ||
55719 | X | 1 | CD |
59435 | X? |
Notes. An X in the second column denotes an SB1 system; the ? indicates objects where there are only hints for an SB1 system. In the last column we point out the new detections (ND), the confirmed detections (CD), and the not reachable companions (NR). The not reachable companions are either potentially very narrow (HD 116114) or outside of our field-of-view (HD 201601).
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