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Fig. A.3.
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Mosaic showing various lines of H I, He I, He II, C III, C IV, and N IV for the reference model mdot0p01/rcsm8e14 at 1 d. In all cases, the x-axis covers from ± 500 km s−1 but the y-axis covers a wide range of normalized fluxes, with very strong narrow emission lines like Hα and much weaker ones like N IV 7122.98 Å.
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