Fig. 1
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Model spectra in the temperature range of B stars, evaluated with TLUSTY+SYNSPEC, showing a few illustrative models between Teff = 11 000 K and 33 000 K for log g = 4.0 evaluated with solar abundances, without rotation or microturbulence. By default, output fluxes evaluated with SYNSPEC are expressed as Eddington fluxes. Notable spectroscopic features of hydrogen and other elements are marked.
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