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Fig. 2


Similar to Fig. 1 but in a narrower wavelength range around the R9 HF line for the extragalactic AGB carbon star Sgr 9 (black line with dots). The red line corresponds to the best fit (log ɛ(F) = 3.75) and black dashed lines are theoretical spectra computed with no F or log ɛ(F) = 3.0, respectively.

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