Table 4
Stellar samples targeting binary companions at ~2 au and 300 au separations.
Embedded | PMS | MS | ||||
---|---|---|---|---|---|---|
MYSOs | Class I | Young OBs | YSOs | O-type | Solar type | |
Sample | 6 | 267 | 16 | 152 | 279 | 454 |
Mass (M⊙) | 8–16 | 0.5–100 (L⊙) | 6.7–39 | 0.25–2.5 | >15 | ~1 |
Method | Interferometry (I) | AO imaging | Interferometry | Aperture masking (AM) | (I+AM) | All combined |
Sensitivity | ΔK ~ 5 | ΔL ~ 4 | ΔK ~ 5 | ΔK ~ 4 | ΔH ~ 5 | ΔV < 3, ΔK < 2.5 |
Binary fraction | 17![]() |
15 ± 2% | 30 ± 11% | 55 ± 6% | 53 ± 5% | 28 ± 2% |
Notes. The binary fractions at those separations are also reported.
References. The references of each class of objects are: This study (MYSOs), Connelley et al. (2008, Class I), GRAVITY Collaboration (2018, Young OBs), Kraus et al. (2011, YSOs), Sana et al. (2014, MS OBs), Raghavan et al. (2010, MS Solar type).
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