\begin{table}%ta.1
\par
\caption {\label{Tab:pulsation}Pseudo-orbital solutions for the Mira S star HD~110~813 (S~UMa) and the
semi-regular carbon star HD~76~221 (X~Cnc), based on the complete data
set but the last two points (see Table~\ref{Tab:Miradata}). 
 }
%\centerline
 {\small\begin{tabular}{llll}
\hline\hline
        & HD 110~813  & HD 76~221 & LSP$^a$\\
\hline
$P_{\rm puls}$ (d) & 222 & 195: & \\
``$P_{\rm orb}$'' (d) & $576\pm1.9$ & $530\pm 8.9$ & 300--1000\\
$e$     & $0.29\pm0.09$ & 0 & 0.08, 0.32--0.37\\
$\omega$ ($^\circ$) & $178\pm17$ & -- & 240--320\\
$T$ (JD$-$2\ts400\ts000) & $52~839\pm23$ & $44541\pm75$\\ 
$K$ (\kms) & $8.5\pm0.6$ & $1.6\pm0.2$ & 1.6--3.1\\
$V_0$ (\kms) & $3.6\pm0.5$ & $-5.9\pm0.1$\\
$f(M)$ (\Msun) & $3.2\times 10^{-2}$ & $(2.3\pm0.9)\;10^{-4}$ & $2\times 10^{-4} {-} 1.3\times 10^{-2}$\\
$a_1 \sin i$ ($10^6$ km) & 64.4 & $11.8\pm1.5$\\
$N$ & 17 & 13\\
$\sigma\rm (O{-}C)$ (\kms) & 1.82 & 0.44\\
\hline
\end{tabular}}
\par
\smallskip
$^a$  The ranges found by \citet{Hinkle-2002} for semi-regular
variables  with long secondary periods. 
\end{table}