Volume 554, June 2013
Article Number A96
Number of page(s) 15
Section Stellar atmospheres
Published online 10 June 2013

Online material

Appendix A: 3D NLTE synthetic line profiles

thumbnail 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

thumbnail Fig. A.2

Same as Fig. A.1, but for HD 84937.

Open with DEXTER

thumbnail Fig. A.3

Same as Fig. A.1, but for HD 140283.

Open with DEXTER

thumbnail Fig. A.4

Same as Fig. A.1, but for G64-12.

Open with DEXTER

© ESO, 2013

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