Fig. 6
Left: identification of the main molecular features formed the observed by LIRIS infrared spectrum of the B component, model atmosphere 3200/5.0/–1.5∗. “Vald” marks the synthetic spectrum computed for atomic line list. H, J, K mark three spectral ranges observed by LIRIS. Right: fit of our synthetic spectra computed with the same model atmosphere, but different oxygen abundances, to the observed SED of G 224-58 B.
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