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Fig. 4.
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Grids of synthetic spectra BSTAR and OSTAR (Lanz & Hubený 2003, 2007) used in our spectroscopic models. Each spectrum is parametrised by log g and T. To describe also critically rotating stars (cf. green points), it was necessary to compute additional ATLAS spectra (Castelli & Kurucz 2003) for low values of log g and T.
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