Free Access
Volume 564, April 2014
Article Number A122
Number of page(s) 11
Section Stellar atmospheres
Published online 17 April 2014

Online material

thumbnail Fig. 4

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).

Open with DEXTER

Table 5

HF line dataa for the R branch (v′ = 1 and v′′ = 0).

Table 6

HF line dataa for the P branch (v′ = 1 and v′′ = 0).

© ESO, 2014

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