Fig. 7
Identified Zr iv (bottom of right panel), Zr v (left panel), and Zr vi (right panel) lines in the FUSE (λ < 1188 Å) and HST/STIS observations of RE 0503−289. The model (thick, red line) was calculated with an abundance of log Zr = −3.5. The dashed green spectrum was calculated without Zr. Prominent lines are marked, the Zr lines with their wavelengths from Tables A.9–A.11.
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