| Issue |
A&A
Volume 578, June 2015
|
|
|---|---|---|
| Article Number | A84 | |
| Number of page(s) | 11 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361/201219577 | |
| Published online | 10 June 2015 | |
Online material
Appendix A: Additional material
 |
Fig. A.1
Coverage of the area around the observed objects, where a binary component within the defined conditions (i.e., ΔK = 2.5, see Chap. 3) can be excluded from the AMBER data. The different colors indicate the areas for the three different baselines and position angles. Upper left: π Sco. Upper right: τ Sco. Lower left: ω Sco. Lower right: χ Oph. |
| Open with DEXTER | |
Properties of the septuple ν Sco.
 |
Fig. A.2
Visibilities and closure phase of π Sco versus wavelength for the H and K bands measured with AMBER on May 6, 2010. |
| Open with DEXTER | |
 |
Fig. A.3
Visibilities and closure phase of π Sco versus wavelength for the H and K bands measured with AMBER on May 10, 2010. |
| Open with DEXTER | |
 |
Fig. A.4
Visibilities and closure phase of ω Sco versus wavelength for the H and K bands measured with AMBER on May 11, 2010. |
| Open with DEXTER | |
 |
Fig. A.5
Visibilities and closure phase of τ Sco versus wavelength for the H and K bands measured with AMBER on May 10, 2010. |
| Open with DEXTER | |
 |
Fig. A.6
Visibilities and closure phase of χ Oph versus wavelength for the H and K bands measured with AMBER on May 6, 2010. |
| Open with DEXTER | |
 |
Fig. A.7
Visibilities and closure phase of χ Oph versus wavelength for the H and K bands measured with AMBER on May 11, 2010. |
| Open with DEXTER | |
© ESO, 2015
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