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Table 3
Best fit observed velocities, in km s-1.
| Line | Haro11A | Haro 11B | Haro 11C | ESO 338-IG04 |
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| Hα | 6227 ± 10 | 6146 ± 5 | 6126 ± 7 | 2859 ± 6 |
| He i | 6242 ± 9 | 6147 ± 6 | 6121 ± 9 | 2856 ± 11 |
| Mg i | ... | 6162 ± 20 | 6128 ± 15 | 2853 ± 20 |
| Na D | ... | 6102 ± 9 | 6158 ± 8 | 2844 ± 14 |
| K i | ... | 6123 ± 20 | 6146 ± 20 | 2830 ± 20 |
Notes. Mgi and K i are measured only from VLT/X-shooter and the uncertainty is therefore larger. The other lines were measured in both VLT/FLAMES and VLT/X-shooter and this represents the weighted average.
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