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Fig. 5

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Temperature structures of the final model atmospheres of G191−B2B (top panel, thick, red line; Rauch et al. 2013, H, He, C, N, O, Al, Si, P, S, Ca, Sc, Ti, V, Cr, Mn, Fe, Co, Ni, Zn, and Ge opacities considered) and RE 0503−289 (bottom panel, thick, red line; Rauch et al. 2014, He, C, N, O, Ca, Sc, Ti, V, Cr, Mn, Fe, Co, Ni, Zn, Ge, Kr, and Xe). The dashed, blue lines show the temperature structures of H+Ba (top) and He+Ba (bottom) models calculated with the same Teff and log g like the final models, respectively. The formation depths (i.e., τ = 1) of the cores of our strategic of the cores of our strategic Ba vi vii lines in FUSE’s wavelength range are marked.

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