Fig. C.1
N IV 6380 for a hot dwarf model (d2v). Black: line profile resulting from our current approach, when manipulating the source functions of EUV background lines with no information on the upper level, as described in the text. Blue: line profile when the EUV two-level-atom source functions are not manipulated. Red: line profile as calculated from our previous FASTWIND version, v10.
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