Fig. B.2.
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Fe II spectrum assuming a 20% contribution from bright sides and 80% contribution from dark sides with minimum χ2 employing the ratios in Sections 3.3 and 4.6, displayed with 33% covering factor after being convolved with a Gaussian kernel with FWHM = 2500 km s−1. The Fe II template corresponds to the CLOUDY simulation associated with logΦ(H) = 20 cm−2 s−1, log(Ptot) = 16 cm−3 K, Z = 20Z⊙ and Vturb = 100 km s−1.
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