Table E.1
Broadening of the FIR lines (in km s-1).
| Broadening | Rotation | ||||||||
|
|
|
||||||||
| [N iii] 57 | [O i] 63 | [O iii] 88 | [N ii] 122 | [O i] 145 | [C ii] 157 | Axis | Vrotation | ||
|
|
|||||||||
| PACS FWHM | 105 | 85 | 125 | 290 | 260 | 240 | |||
|
|
|||||||||
| Haro 2 | n.a. | 90 | 140 | n.a. | n.a. | – | – | – | |
| Haro 3 | 100 | 90 | 110 | – | – | – | NEE–SWW | ±30 km s-1 | |
| Haro 11 | 160 | 130 | 200 | 200 | 100 | 160 | N–S | ±50 km s-1 | |
| He 2-10 | 160 | 100 | 170 | – | – | – | NE–SW | ±20 km s-1 | |
| HS 1330+3651 | n.a. | – | 150 | n.a. | n.a. | – | – | – | |
| II Zw 40 | n.a. | 80 | 110 | – | – | – | N–S | ±30 km s-1 | |
| Mrk 1089 | n.a. | 80 | 130 | – | – | – | NNE–SSW | ±80 km s-1 | |
| Mrk 153 | n.a. | 80 | 120 | n.a. | n.a. | – | NE–SW | ±30 km s-1 | |
| Mrk 930 | n.a. | 120 | 120 | – | – | – | N–S | ±30 km s-1 | |
| NGC 1140 | n.a. | 100 | 100 | – | – | – | NE–SW | ±40 km s-1 | |
| NGC 1569 | n.a. | 80 | 100 | n.a. | n.a. | – | – | – | |
| NGC 1705 | n.a. | – | 100 | n.a. | n.a. | – | – | – | |
| NGC 2366 | n.a. | 80 | 70 | n.a. | n.a. | – | – | - | |
| NGC 4214 | n.a. | 80 | 80 | – | – | – | – | - | |
| SBS 1533+574 | n.a. | – | 80 | n.a. | n.a. | – | – | – | |
| UM 448 | n.a. | 150 | 150 | – | 80 | 150 | NNE–SSW | ±60 km s-1 | |
| IC 10 | n.a. | 90 | 70 | – | – | – | – | - | |
| LMC | 150 | 150 | 150 | 100 | 100 | – | – | – | |
| SMC | n.a. | 150 | 150 | n.a. | n.a. | – | – | – | |
| NGC 4449 | n.a. | 90 | 90 | – | – | – | – | – | |
| NGC 5253 | n.a. | 60 | 90 | – | – | – | NE–SW | ±30 km s-1 | |
| NGC 6822 | n.a. | 100 | 80 | – | – | – | – | – | |
Notes. The broadening (or intrinsic line width) is given as the observed FWHM subtracted by the instrumental FWHM. Uncertainties are on the order of 20%. We indicate the broadening of the spaxel where the emission peaks. This value can be higher elsewhere because of rotation or instrumental effects (uncentered point-source).
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