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$a_1 \sin i$ (Gm) & 125.585 +/- 0.170 $a_2 \sin i$ (Gm) & 189.35 +/- 2.21 ${\cal M}_1 \sin^3 i$ (${\cal M}_\odot$) & 0.9627 +/- 0.0248 ${\cal M}_2 \sin^3 i$ (${\cal M}_\odot$) & 0.63850 +/- 0.00910 $\sigma_{o-c}$ SOPHIE (km/s) & 0.0394/0.202 $\sigma_{o-c}$ Ancient (km/s) & 0.84/1.24 Remark: Orbit obtained from high-precision measurements derived from 9 CCD-spectra reduced with TODMOR, and from ancient measurements collected by McAlister et al. (1995).The orbital elements were derived adding a systematic shift $D_0 = 1.9108 +/- 0.0483$ km/s to the ancient measurements. Taking into account 3 astrometric observations performed with long-base interferometer, the masses of the components are 1.1033 +/- 0.0292 and 0.7317 +/- 0.0113, respectively. The parallax of the binary is 36.629 +/- 0.220 mas. References: McAlister, H.A., Hartkopf, W.I., Mason, B.D., Fekel, F.C., Tokovinin, A.A., Griffin, R.F., and Culver, R.B. 1995, AJ, 110, 366 |
omega was originally 0 in the publication. |
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