Table 4
Properties of extended emission-line regions.
| Source | [OIII] size | FWH Mavg | FWH M max | Δv | v/σavg | v/σmax | Kin. class | |
| [kpc×kpc] | [km s-1] | [km s-1] | [km s-1] | |||||
|
|
||||||||
| BRL 0128−264 | 16.8 ± 3.9 × 5.9 ± 2.7 | 1300 ± 124 | 1910 ± 182 | 1550 ± 148 | 1.4 ± 0.2 | 1.0 ± 0.2 | BB | |
| MRC 0156−252 | 68.6 ± 3.6 × 22.5 ± 3.6 | 660 ± 21 | 990 ± 31 | 1220 ± 38 | 2.3 ± 0.1 | 1.5 ± 0.1 | BB | |
| USS 0211−1221 | 17.0 ± 4.0 × 6.8 ± 1.5 | 200 ± 32 | 240 ± 39 | 124 ± 20 | 0.6 ± 0.2 | 0.4 ± 0.2 | BB | |
| MRC 0251−273 | 24.1 ± 3.3 × 14.0 ± 2.9 | 670 ± 54 | 450 ± 36 | 780 ± 64 | 0.7 ± 0.4 | 0.6 ± 0.2 | Irr | |
| RC J0311+0507 | 11.4 ± 3.6 × 10.4 ± 3.2 2 | 510 ± 20 | 680 ± 27 | 200 ± 8 | 0.5 ± 0.1 | 0.3 ± 0.1 | BB | |
| MP J0340−6507 | 23.1 ± 5.8 × 13.6 ± 5.4 | 900 ± 137 | 1250 ± 190 | 420 ± 64 | 0.5 ± 0.1 | 0.4 ± 0.1 | Irr | |
| PKS 0529−549 | 17.6 ± 3.0 × 9.6 ± 2.7 | 610 ± 36 | 820 ± 48 | 470 ± 28 | 0.9 ± 0.1 | 0.7 ± 0.1 | Irr | |
| sTN J1112−2948 | 45.9 ± 3.3 × 9.7 ± 2.9 | 437 ± 23 | 780 ± 35 | 610 ± 27 | 1.6 ± 0.2 | 0.9 ± 0.2 | BB | |
| TXS 1113−178 | 9.2 ± 2.3 × 8.3 ± 2.3 | 790 ± 70 | 1130 ± 100 | 530 ± 47 | 0.8 ± 0.3 | 0.6 ± 0.1 | BB | |
| 3C 257 | 16.7 ± 3.0 × 9.1 ± 2.8 | 1010 ± 88 | 1410 ± 123 | 400 ± 35 | 0.5 ± 0.1 | 0.3 ± 0.1 | Irr | |
| USS 1243+036 | 37.3 ± 2.8 × 6.7 ± 1.8 | 880 ± 22 | 3180 ± 57 | 1950 ± 35 | 2.6 ± 0.2 | 0.7 ± 0.1 | BB | |
| TN J1338−1942 | 9.4 ± 3.3×6.9 ± 2.7 | 994 ± 47 | 1510 ± 71 | 850 ± 40 | 1.0 ± 0.3 | 0.7 ± 0.1 | Irr | |
| USS 1410−001 | 40.6 ± 3.1×13.8 ± 2.9 | 780 ± 52 | 1340 ± 89 | 710 ± 47 | 1.1 ± 0.1 | 0.6 ± 0.1 | BB | |
| MRC 1558−003 | 40.6 ± 3.9×21.5 ± 3.9 | 763 ± 82 | 1050 ± 112 | 730 ± 78 | 1.1 ± 0.1 | 0.8 ± 0.1 | Irr | |
| USS 1707+105 | 24.6 ± 3.1×4.9 ± 2.0 | 920 ± 87 | 1900 ± 179 | 680 ± 64 | 0.8 ± 0.1 | 0.4 ± 0.2 | Irr | |
| 3C 362 | 30.5 ± 4.9×13.6 ± 4.7 | 1030 ± 122 | 1625 ± 192 | 720 ± 85 | 0.8 ± 0.1 | 0.5 ± 0.2 | Irr | |
| MP 1758−6738 | 31.0 ± 3.2×14.8 ± 2.9 | 700 ± 75 | 1060 ± 114 | 660 ± 71 | 1.1 ± 0.2 | 0.7 ± 0.1 | BB | |
| TN J2007−1316 | 10.1 ± 3.0×5.9 ± 1.4 | 970 ± 140 | 1200 ± 173 | 100 ± 733 | 0.1 ± 0.1 | 0.1 ± 0.1 | BB | |
| MRC 2025−218 | 27.0 ± 4.2×8.9 ± 3.4 | 1060 ± 97 | 1707 ± 157 | 620 ± 57 | 0.7 ± 0.2 | 0.4 ± 0.1 | Irr | |
| MRC 2104−242 | 60.5 ± 2.8×18.6 ± 2.3 | 670 ± 27 | 1237 ± 52 | 930 ± 39 | 1.6 ± 0.2 | 0.9 ± 0.2 | Irr | |
| 4C 23.56 | 49.3 ± 3.4×21.8 ± 3.1 | 640 ± 21 | 1060 ± 36 | 1010 ± 40 | 1.8 ± 0.2 | 1.2 ± 0.1 | BB | |
| NVSS J2135−3337 | 17.8 ± 1.8×10.5 ± 1.8 | 510 ± 25 | 1140 ± 43 | 410 ± 59 | 1.0 ± 0.2 | 0.4 ± 0.2 | BB | |
| MG 2144+1928 | 37.6 ± 4.4×10.7 ± 2.7 | 700 ± 73 | 1930 ± 164 | 790 ± 28 | 1.3 ± 0.1 | 0.5 ± 0.2 | Irr | |
| TN J2254+1857 | 21.1 ± 3.2×12.1 ± 2.8 | 850 ± 63 | 1483 ± 109 | 800 ± 59 | 0.5 ± 0.1 | 0.3 ± 0.2 | BB | |
| MG 2308+0336 | 30.5 ± 3.0×12.5 ± 2.7 | 850 ± 53 | 1440 ± 90 | 1200 ± 75 | 1.7 ± 0.2 | 1.0 ± 0.2 | BB | |
Notes. The [OIII] size is the full projected length of the emission-line region along the major and minor axis, respectively, and deconvolved with the size of the seeing disk. We only list galaxies of type “BB” (bipolar velocity fields akin to back-to-back outflows) or “Irr” (irregular kinematics).
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