Fig. 5
Spectrum synthesis of the C I lines at 6007.176 and 6010.675 Å for IRAS 22223+4327. The black spectrum is the observed HERMES spectrum; the coloured spectra represent synthetic spectra with different C abundances. The red line represents the determined C abundance; the green and blue spectra represent synthetic spectra with a C abundance of −0.2 dex and +0.2 dex, respectively.
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