Open Access

Fig. 10.

image

Same as Fig. 6, with other processes. First column: effect of removing dust. We also remove the fine-structure level to simplify the interpretation. Second column: spectra with and without gas motion in the galaxy. Infilling effects give complex shapes to the second and seventh rows. Third column: comparison of fiducial spectra with spectra with neither gas motion, dust, scattering, nor fine-structure level.

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