Fig. 7.
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Contribution and distribution of the star-forming gas. Left: Averaged contribution of the star-forming gas (dot-dashed magenta line) and non star-forming gas (dashed brown line) to the total [CII] emitting gas (orange line). The shaded areas enclose 95% of different results obtained by different galaxy orientations. Right: SFR density map for a TNG50 galaxy at z = 5. The box goes out to ∼40 kpc or ∼R200 from the central galaxy.
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