Fig. 2
Top: comparison of two SEDs from He+Ga composed model-atmospheres
(, log g = 7.5, 100 times
solar Ga abundance), on the one hand calculated with a classical (thick, blue in the
online version) and on the other hand with a statistical (thin, red) Ga model atom.
The SEDs are convolved with a Gaussian (FWHM = 0.06 Å) to simulate the FUSE resolution.
Inset: wider wavelength range (statistical Ga model atom only).
Bottom: 
illustrates the deviation between the
two fluxes.
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