| Issue |
A&A
Volume 566, June 2014
|
|
|---|---|---|
| Article Number | A88 | |
| Number of page(s) | 11 | |
| Section | Stellar atmospheres | |
| DOI | https://doi.org/10.1051/0004-6361/201323264 | |
| Published online | 19 June 2014 | |
Online material
 |
Fig. 2
Left: from top to bottom, observed (black) squared visibility amplitudes, UD diameters predicted from our data (blue) and from the best-fit PHOENIX model (red), closure phases in degrees, and normalized flux of ϵ Oct obtained on 2012 Jun. 25. Right: same as left, but for data obtained on 2012 Aug. 02. |
| Open with DEXTER | |
 |
Fig. 3
Left: from top to bottom, observed (black) squared visibility amplitudes, UD diameters predicted from our data (blue) and from the best-fit PHOENIX model (red), closure phases in degrees, and normalized flux of NU Pav obtained on 2012 Aug. 02. Right: same as left, but for data from ψ Peg obtained on 2012 Jun. 16. |
| Open with DEXTER | |
 |
Fig. 4
Left: from top to bottom, observed (black) squared visibility amplitudes, UD diameters predicted from our data (blue) and from the best-fit PHOENIX model (red), and closure phases in degrees of γ Hya obtained on 2013 Mar. 16. Right: same as left, but obtained with the MR-K 2.3 μm setting. |
| Open with DEXTER | |
© ESO, 2014
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