Table 4.
Trial FOTEL orbital solutions based on all 151 phdia and asTODCOR RVs and a solution for the 65 RVs of the Hα emission wings measured in SPEFO.
| Element | Binary | emis. wings Hα |
|---|---|---|
| P (d) | 33.77458 ± 0.00079 | 33.77458 fixed |
| Tsuper. c. | 55487.657 ± 0.020 | 55492.53 ± 0.49 |
| e | 0.0 assumed | 0.0 assumed |
| K1 (km s−1) | 7.76 ± 0.56 | 9.47 ± 0.88 |
| K2 (km s−1) | 81.75 ± 0.17 | – |
| K2/K1 | 0.0949 ± 0.0063 | – |
| γ1 (km s−1) | −13.46 ± 0.18 | −11.33 ± 0.85 |
| γ2 (km s−1) | −13.04 ± 0.24 | – |
| γ3 (km s−1) | −13.10 ± 1.38 | – |
| γ4 (km s−1) | −13.69 ± 0.25 | −13.13 ± 0.74 |
| γ3T1 (km s−1) | −0.39 ± 0.37 ( * ) | – |
| γ3T2 (km s−1) | −0.20 ± 0.33 ( * ) | – |
| rms (km s−1) | 1.138 | 2.71 |
Notes. The epoch of superior conjunction of star 1 is in RJD, rms is the rms error of 1 observation of unit weight. ( * )We note that the asTODCOR RVs derived using the KOREL templates refer to zero systemic velocity.
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