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Fig. A.6
Best-fit model for MPG 113 (in red) compared with observed spectra (in black): the STIS spectrum (upper left) and the FLAMES+ UVES spectra (upper right). The bottom plot shows a comparison with the UVES spectrum for spectral regions around O iiiλ5592 (left), C iiiλ5696 (middle), and He iλ5876 (right).
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