Table C.2
Orbital solutions for the comparison star HR 96.
| Element | Hube (1983) | Our new | ||||
|
|
||||||
| P (d) | 48.2905(42) | 48.2884(15) | ||||
| T periastr. | 45 248.12(60)⋆ | 45 248.29(35) | ||||
| T super.c. | 45 260.12 | 45 260.24 | ||||
| T RVmax. | 45 250.43 | 45 250.58 | ||||
| e | 0.384(29) | 0.376(25) | ||||
| ω (deg.) | 320.0(6.8) | 321.0(2.9) | ||||
| K1 (km s-1) | 30.1(1.0) | 29.02(74) | ||||
| γDDO old (km s-1) | – | + 9.37(56) | ||||
| γHRM (km s-1) | – | + 1.8(2.6) | ||||
| γDDO new (km s-1) | – | −0.23(39) | ||||
| γDAO (km s-1) | +3.41(74) | +3.22(73) | ||||
| rms (km s-1) | not given | 2.10 | ||||
| No. of RVs | 25 | 36 | ||||
Notes.
The epoch given by Hube (1983), 45 240.60(60) is an obvious misprint and cannot reproduce the phase plot in his Fig. 1. We quote his period with the error derived also from all 36 RVs, which he fixed in the above reproduced solution based on the DAO RVs only. All epochs are in RJD; rms is the rms of one observation of unit weight.
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