Volume 564, April 2014
|Number of page(s)||11|
|Published online||17 April 2014|
Observed spectra in black and synthetic spectra in red for the B3-BW-B6 stars. The three Zr-lines, the [O i]-line, the OH-lines, and the HF-line used are marked. The exact wavelengths are listed in Table 4. The OH-lines with obvious cosmic hits were excluded from the fit. Note the different flux scales. An example of the HF-line in the re-analyzed BMB-I-IV can be found in Cunha et al. (2008).
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© ESO, 2014
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