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Table 4
Properties of the detected stellar companions.
| Primary name | Separation | PA | ΔCH4s | ΔKs | Massa | |
| (as) | (deg) | (mag) | (mag) | (M⊙) | ||
|
|
||||||
| HIP 42334 | 3.176 ± 0.007 | 11.52 ± 0.12 | ... | 8.2 ± 0.1 | 0.07–0.11 | |
| HIP 104365 | 9.545 ± 0.006 | 15.27 ± 0.04 | 7.4 ± 0.1 | ... | 0.09–0.13 | |
| 9.595 ± 0.006 | 14.27 ± 0.04 | 7.4 ± 0.1 | ... | 0.09–0.14 | ||
Notes.
(a)
The mass range was estimated using the DUSTY evolutionary models (Chabrier et al. 2000) taking into account the uncertainties on the distance, on the magnitude of the primary, on the contrast of the companion, and on the age of the system.
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