Table 6.
General properties of the ionised nebulae.
| Source | dmax | rmax | Nature of prominent | Outside | Ref. |
|---|---|---|---|---|---|
| [kpc] | [kpc] | ionised features | cones? | ||
| (1) | (2) | (3) | (4) | (5) | (6) |
| J0802+25 | 38 | 21 | Low surface brightness large (∼38 kpc) asymmetric nebula | Yes | F18 |
| J0841+01 | 42 | 21 | Ionisation cone or giant (∼8 kpc) bubble? | Yes | S18 |
| bent arm tracing eastern radio source across 12 kpc | |||||
| tidal features, TDGC | |||||
| J0853+38 | 100 | 70 | Bent arms tracing the radio source across > 60 kpc | Yes | |
| SF in spiral arms; distant patches | |||||
| J0907+46 | 68 | 46 | Nebula (∼13 kpc) tracing the inner radio source | No? | |
| tidal tail, TDGC | |||||
| J0945+17 | 25 | 15 | Giant bubble candidate (∼10 kpc), filaments | No? | S18 |
| J1000+12 | 112 | 90 | Blob, jet-like feature (∼9 kpc), giant bubble candidate (∼10 kpc) | No | J19 |
| extension tracing the NW radio source, tidal tail, TDGC | |||||
| J1316+44 | 92 | 53 | Tidal bridge, distant patches | Yes | |
| widely spread SF in host galaxy | |||||
| J1356+10 | 119 | 92 | Giant bubbles and shells (∼12–30 kpc) | Yes | G12,J19 |
| large asymmetric nebula (∼70 kpc), tidal brige/filament, TDGC | |||||
| Teacup | 132 | 90 | Giant bubble (∼10 kpc), giant (∼115 kpc × 87 kpc) nebula | Yes | K12,VM18 |
| arc (edge brightened cavity?), filament (∼30 kpc), distant patches | |||||
| J1437+30 | 22 | 12 | SF knot, low surface brightness asymmetric ∼12 kpc nebula | Yes | F18 |
Notes. (2) dmax: maximum distance in kpc between detected ionised gas features; (3) rmax: distance in kpc from the QSO2 nucleus to the most distant ionised gas feature detected; (4) morphological classification of prominent ionised features; (5) considering whether there is gas outside the putative QSO2 ionisation cones; (6) J0948+25, J1108+06 and J1517+33 are not in this table because there are no emission line images available.
References. G12: Greene et al. 2012; K12: Keel et al. (2012); H15: Jarvis et al. (2019); S18: Storchi-Bergmann et al. (2018); V18: Villar-Martín et al. (2018); F18: Fischer et al. (2018); J19: Jarvis et al. (2019).
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