Table 2: Parameters of the best orbital solution.
\begin{displaymath}\begin{tabular}{cr@{~$\pm$~}l\vert cr@{~$\pm$~}l} \hline \hli... ...{{\rm Sb}}$ ($M_\odot$) & 0.61 & 0.17 \\ \hline \end{tabular}\end{displaymath}
a The uncertainty on the derived quantities include
that induced by the distance estimate.

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