A theoretical investigation of far-infrared fine structure lines at z > 6 and of the origin of the [O III]88 μm/[C II]158 μm enhancement

Open Access

Fig. 4.

[N II] line emission maps obtained with the Solar model (top panels), the High-z model (middle panels), and the Dwarfs model (bottom panels). The right panels are zoomed-in images of the main disc and surrounding area. The white dashed circles mark the extent of R_vir of PONOS.

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