Fig. 4
Observed Sr line of S 11-04 at 4215 Å (dots). The red solid line shows the synthetic spectra for the abundance derived by our analysis. The blue dashed lines are the spectra calculated after changing the Sr abundance by ±0.5 dex. The green dot-dashed line shows a spectrum calculated as the equivalent width obtained by Tafelmeyer et al. (2010) is reproduced.
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