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Table 3.

Outflow properties.

NW SE Sect.
Ionised component

Rout (kpc) 4 6 4.2.3
Ne (cm−3) 1480 ± 870 136 ± 45 7
Te (×104 K) 1.8 ± 0.4 2.04 ± 0.01 7
vout (km s−1) −740 ± 20 +460 ± 12 4.2.1
L[O III] (×1040 erg s−1) 5.9 ± 0.5 2.4 ± 0.3 9
(M yr−1) 0.05 ± 0.03 0.07 ± 0.02
(×1040 erg s−1) 0.8 ± 0.2 0.4 ± 0.1
[O III] (×1033 dyne) 0.23 ± 0.08 0.20 ± 0.03
LHβ (×1041 erg s−1) 1.4 ± 0.1 0.61 ± 0.09
(M yr−1) 1.2 ± 0.7 3.0 ± 1.5
(×1041 erg s−1) 1.8 ± 1.3 2.0 ± 1.3
Hβ (×1033 dyne) 5.1 ± 2.5 4.4 ± 2.2

Neutral component

Rout (kpc) ≳4 ≳2 4.2.3
Ω 2π* 2π*
vout (km s−1) ( − 550 ± 35); (−1150 ± 105) −530 ± 30 4.2.2
Cf (0.46 ± 0.15); (0.15 ± 0.11) 0.5 ± 0.2 6
log(NH) (20.0 ± 0.1); (19.9 ± 0.1) 20.0 ± 0.1 6
out (M yr−1) (5 ± 4); (17.5 ± 3) 5 ± 4 9
(×1041 erg s−1) (4 ± 3); (70 ± 25) 4 ± 2
(×1033 dyne) (15 ± 13); (123 ± 15) 15 ± 11

Total (neutral+ionised)

out (M yr−1) 24 ± 5 8 ± 4 9
(×1041 erg s−1) 76 ± 25 6 ± 2
(×1033 dyne) 143 ± 20 19 ± 10
μ 0.3 0.7
0.17 0.08
0.004 0.004
/(Lbol/c) 2 3

Notes. [O III] and Hβ luminosities are corrected for extinction using the values reported in Table 1. For the neutral phase of the NW outflow, we report the derived properties for each of the two kinematic components described in Sect. 6. Mass-loading factors (μ) and kinetic power expected for stellar processes () are derived using the SFR reported in Yuan et al. (2018). AGN bolometric luminosities from [O III] line flux: erg s−1, erg s−1. The asterisk indicates the assumed value for the solid angle of the wind. Only statistical errors are reported for the outflow energetics (larger systematic uncertainties, e.g. due to an incorrect assumption on geometrical configurations, might affect our individual measurements; see e.g. Perna et al. 2015b).

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