Table 8.
Fit parameters of all the lines considered.
| Line | K (km s−1) | ϕ0 | γ (km s−1) |
 |
|---|---|---|---|---|
| Pa 10 | 125.1 ± 9.6 | 0.38 ± 0.01 | −149.1 ± 7.4 | 1.40 |
| Pa 11 | 129.0 ± 9.7 | 0.38 ± 0.01 | −137.5 ± 7.4 | 2.01 |
| Pa 12 | 123.8 ± 9.5 | 0.39 ± 0.01 | −151.1 ± 6.6 | 0.67 |
| He 5875 Å | 53.4 ± 10.0 | 0.38 ± 0.02 | −184.5 ± 6.6 | 0.67 |
| He 7065 Å | 56.9 ± 8.7 | 0.46 ± 0.03 | −193.6 ± 6.6 | 1.38 |
| He 6678 Å | 105.1 ± 12.6 | 0.39 ± 0.02 | −134.9 ± 9.5 | 1.30 |
| O 7774 Å | 108.4 ± 10.9 | 0.34 ± 0.01 | −101.9 ± 6.7 | 2.23 |
| O 8446 Å | 18.6 ± 2.2 | 0.17 ± 0.01 | −4.5 ± 1.3 (a) | 1.4 |
| 26.7 ± 8.9 | 0.08 ± 0.06 | 54.1 ± 6.5 (b) | 0.7 |
Notes. The two O I 8446 Å transition are from EMMI and cross-correlated X-shooter analyses, respectively (Figs. 14 and 15). ϕ0 is in orbital phase units.
Fit parameters obtained from the velocities shown in Fig. 15. All the velocities have been heliocentric corrected only.
Fit parameters obtained from the velocities shown in Fig. 14. All the velocities have been obtained by measuring the deep absorption in the core of the line.
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