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Fig. 5


Best fits (continuous curve) of the spectral ranges 3727.73728.5 Å and 3795.63797.1 Å (top row), where the investigated Ru i, Tm ii, Gd ii, and Ho ii lines are located; Ir i 3800 Å and Os i 4260 Å (bottom row) in the observed spectrum of HE 22524225 (bold dots). The dotted curves show the synthetic spectrum with no relevant element in the atmosphere. The dashed curve in the top left panel shows the effect of a 0.2 dex lower Ru abundance on the synthetic spectrum.

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