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Fig. 6

image

STIS observation of G191−B2B (gray) compared with synthetic line profiles of In V λ 1334.123 Å and In V λ 1339.599 Å calculated with four In abundances: without (thin blue line), with 1000 times (thick red), 10 000 times (short-dashed violet), and 100 000 times solar abundance (long-dashed green).

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