Fig. 20.

Inflow in ESO 320-G030 observed in the far-IR [O I] 63 μm line and OH doublets. The gray vertical lines indicate the position of the two components of the OH doublets (blended within a single feature in the case of OH 71 μm in panel g), and the vertical arrows in panel c indicate the position of the 18OH 79 μm doublet components. OH is modeled with the same components as derived from H2O: the core (dashed blue lines), the nuclear disk (dashed green) and the envelope (dashed gray); red is total. The inflow is simulated in the envelope component (see Sect. 4.2). The model also includes the contribution by 18OH, NH3, and H2O in panels c, e, and f–g, respectively (see Appendix A).
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