| Issue |
A&A
Volume 554, June 2013
|
|
|---|---|---|
| Article Number | A96 | |
| Number of page(s) | 15 | |
| Section | Stellar atmospheres | |
| DOI | https://doi.org/10.1051/0004-6361/201321406 | |
| Published online | 10 June 2013 | |
Online material
Appendix A: 3D NLTE synthetic line profiles
 |
Fig. A.1
Observed line profiles (black solid lines) and best-fit 3D, NLTE synthetic profiles (red solid lines) for HD 19445. Below each panel is shown the flux residual (observed-synthetic) in per cent. When vrotsini has not been solved for, the value has been fixed to 3.0. Only lines with Wλ < 50 mÅ have been included to estimate the vrotsini-values used for analysis of Li line to determine the Li isotopic ratio. |
| Open with DEXTER | |
 |
Fig. A.2
Same as Fig. A.1, but for HD 84937. |
| Open with DEXTER | |
 |
Fig. A.3
Same as Fig. A.1, but for HD 140283. |
| Open with DEXTER | |
 |
Fig. A.4
Same as Fig. A.1, but for G64-12. |
| Open with DEXTER | |
© ESO, 2013
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