Table 6.
Outflow parameters derived for the LINERs with a detection, including NGC 1052 (see Cazzoli et al. 2022).
| Galaxy | vOF, ion | ROF, ion | MOF, ion | ṁOF,ion | EOF, ion | ĖOF,ion | ĖOF,ion/Lbol | ne |
|---|---|---|---|---|---|---|---|---|
| (km s−1) | (pc) | (M⊙) | (M⊙ yr−1) | (erg) | (erg s−1) | (cm−3) | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| NGC 1052 | 655 | 792 | 1.6 ± 0.6 × 105 | 0.36 ± 0.27 | 1.3 ± 0.9 × 1053 | 8.8 ± 3.5 × 1040 | 0.01 | 360 |
| NGC 3226 | 138 | 242 | 1.5 ± 0.1 × 105 | 0.26 ± 0.05 | 9.0 ± 3.1 × 1052 | 1.7 ± 0.6 × 1040 | 0.008 | 591 |
| NGC 3245 | 580 | 322 | 2.1 ± 0.1 × 104 | 0.11 ± 0.03 | 0.5 ± 0.4 × 1051 | 1.2 ± 0.7 × 1040 | 0.006 | 787 |
| NGC 4278( * ) | 241 | 122 | 2.0 ± 0.5 × 103 | 0.004 ± 0.001 | 4.5 ± 2.6 × 1049 | 7.2 ± 1.7 × 1037 | 0.00002 | 314 |
| NGC 4438 | 213 | 307 | 1.90 ± 0.01 × 103 | 0.004 ± 0.001 | 1.0 ± 0.6 × 1051 | 2.7 ± 1.4 × 1038 | 0.0001 | 710 |
| NGC 4750 | 191 | 318 | 4.2 ± 0.1 × 104 | 0.08 ± 0.02 | 3.8 ± 1.0 × 1052 | 7.5 ± 2.7 × 1039 | 0.02 | 686 |
Notes. Columns indicate: (1) object; (2) maximum velocity of the component associated with the outflow; (3) extension of the outflow; (4) mass of the ionised outflow; (5) mass outflow rate; (6) kinetic energy; (7) kinetic power of the outflow; (8) energy rate and (9) mean electronic density. ( * )indicates that the MOF, ion was estimated with the Hβ luminosity instead of Hα. See Sect. 4.3 for more details on the calculations.
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