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Table 4.

Outflow properties measured from the [O III]λ5007 Å emission line.

ID log ne ( * ) Mout × 106 Rout PA vout out log Ėkin ξ
[cm−3] [M] [kpc] [ ° ] [km s−1] [M yr−1] [erg s−1] [%]
(1) (2) (3) (4) (5) (6) (7) (8) (9)
J1100 63 42.02 0.0148
J1356 197 | 200 −631 41.32 0.0060
J1430 65 | 198 −760529 41.13 0.0020
J1509 320 −1289 41.18 0.0012

ID log ne ( * *) Mout × 106 Rout PA vout out log Ėkin ξ
[cm−3] [M] [kpc] [ ° ] [km s−1] [M yr−1] [erg s−1] [%]

J1100 63 41.03 0.0015
J1356 197 | 200 −631 40.58 0.0011
J1430 65 | 198 −760529 40.90 0.0011
J1509 320 −1289 40.61 0.0003

Notes. (1) Object ID; (2) electron density; (3) mass of the outflowing gas; (4) maximum outflow radius; (5) position angle of the outflow; (6) outflow velocity measured from the velocity maps (negative velocities correspond to vel05 and positive to vel95); (7) mass outflow rate computed as 3  ×  vout × Mout/Rout; (8) outflow kinetic energy calculated as , with σ being the velocity dispersion, measured as FWHM = 2.355/σ, with FHWM = W80/1.09; (9) coupling efficiency (ξ = Ėkin/Lbol).

( * )Electron densities computed from the [S II]λλ6716, 6731 doublet ([S II]).

( * *)Electron densities computed using the trans-auroral lines (TA). Two values of Rout, PA, and vout are reported for J1356 and J1430 because the redshifted side of the outflow is also detected. For them, the outflow mass rates, kinetic powers, and coupling efficiencies are calculated independently for the blueshifted and redshifted sides of the outflow, and then added.

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