Table 3.
Summary of the outflowing systems.
| System | Detection | Location [pc] | Extent [pc] | vr [km s−1] | σ [km s−1] |
|---|---|---|---|---|---|
| H0 | Hβ, Hα, [O III] | < 2.1 | 4.6 ± 0.6 | −211 ± 22 | 218 ± 7 |
| O1 | Hβ, Hα, [O III] | < 0.85 | < 1.7 | −144 ± 5 | 165 ± 17 |
| O2 | Hβ, Hα, [O III] | < 0.85 | < 1.7 | −560 ± 20 | 251 ± 31 |
| L1 | Ly-α | – | – | −278 ± 43 | 17 ± 6 |
| L2 | Ly-α | – | – | −1118 ± 2 | 41 ± 5 |
Notes. The only component that we spatially resolve are the Hα and Hβ core components in the AGN spectrum (Fig. 1). Their kinematic parameters listed here correspond to those of the core component of the two-component 
integrated two-component fit described in Sect. 4.1. The [O III] emitters O1 and O2 are spatially unresolved. Their maximum offset and size equals the systematic uncertainty of our measurement. For the Ly-α absorbers, the spatial extent is not constrained.
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