Table 4
Galaxy properties: escape velocities and disks thickness.
| ID1 | v esc | Vw/vesc | hz(Hα) | hz(NaD) |
| IRAS | km s-1 | pc | pc | |
| (1) | (2) | (3) | (4) | (5) |
|
|
||||
| F01159-4443 (N) | 397 | 0.3 | 35 ± 7 | ··· |
| F01341-3735 (N) | 332 | 0.3 | 30 ± 5 | ··· |
| F04315-0840 | 232 | 1.4 | 218 ± 44 | ··· |
| F05189-2524 | 258 | 1.4 | 1757 ± 352 | ··· |
| F06206-6315 | 389 | 4.2 | 187 ± 37 | ··· |
| F06259-4780 (N) | 286 | 1.4 | 227 ± 45 | ··· |
| F06259-4780 (C) | ··· | ··· | 246± 49 | 2759 ± 552 |
| F06592-6313 | 251 | 2.6 | 135 ± 27 | ··· |
| F07027-6011 (N) | 416 | 0.7 | 110 ± 22 | ··· |
| F07027-6011 (S)‡ | 275 | 0.6 | 248 ± 50 | 2431 ± 486 |
| F07160-6215 | 502 | 1.4 | 100 ± 20 | ··· |
| F09437+0317 (N) | ··· | ··· | 111 ±22 | 713 ± 143 |
| F09437+0317 (S) | ··· | ··· | 46 ± 7 | 1879 ± 376 |
| F10015-0614 | 492 | 0.6 | 87 ± 17 | ··· |
| F10038-3338 | 203 | 1.0 | 1969 ± 394 | ··· |
| F10257-4339 | 318 | 0.8 | 109 ± 22 | ··· |
| F10409-4556‡ | 409 | 1.2 | 57 ± 11 | 1390 ± 278 |
| F10567-4310 | 401 | 0.3 | 32 ± 6 | ··· |
| F11255-4120 | 303 | 0.9 | 56 ± 11 | ··· |
| F11506-3851‡ | 393 | 0.2 | 35 ± 6 | 1541 ± 308 |
| F12043-3140 (S) | ··· | ··· | 347 ± 69 | 1315 ± 263 |
| F12115-4656 | ··· | ··· | 40 ± 8 | 1845 ± 369 |
| 12116-5615‡ | 159 | 3.2 | 1779 ± 355 | ··· |
| F13001-2339 | 600 | 0.6 | 828 ± 166 | ··· |
| F13229-2934 | 332 | 0.2 | 191 ± 38 | ··· |
| F14544-4255 (E) | ··· | ··· | 142 ± 28 | 1287 ± 257 |
| F18093-5744 (S) | ··· | ··· | 122 ± 24 | 1261 ± 252 |
| F21453-3511 | 169 | 0.8 | 350 ± 70 | ··· |
| F22132-3705 | ··· | ··· | 43 ± 9 | 922 ± 184 |
| F23128-5919 | 292 | 1.6 | 200 ± 40 | ··· |
Notes. Column (1): ID. Column (2): escape velocity for those galaxies hosting a GW (Table 1) as derived in Sect. 4.6. Column (3): the ratio between the inclination-corrected wind median velocities (Table 3) and the escape velocity. Columns (4) and (5): vertical ionized and neutral gas disk heights traced via Hα (narrow component, Bellocchi et al. 2013) and NaD, respectively (Sect. 4.8). As in Table 3, the symbol:
, marks the galaxies for which a two-components NaD modeling have been done (Sect. 2.3). We assumed a conservative 20% systematic error for all the hz values.
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