\begin{table}%t1
\caption{\label{table:1}Relevant data for our sample of S-MS~stars.}
%\centering
\par
\begin{tabular}{l c c c c r r c c c}         
\hline\hline\noalign{\smallskip}
Source   & Spectral type & Var. type &  Distance$^a$   & Bol. Magnitudes$^b$ &   Mass Loss   &  v$_{e}$ &   Ref.$^c$ &  I. $-$ E. & dust/gas \\
Name   & & (GCVS) &  (kpc)   & (Paper II) &   (M$_{\odot}$/yr)  & km/s &   &   & ratio \\
\hline
\object{S Cas}  & S3,4e$-$S5,8e & Mira &   0.85$^B$    & $-$5.71 &   1.02E$-$5 & 20.5   &   R & I & 2.16E$-$4  \\
\object{W Aql}  & S3,9e$-$S6,9e & Mira &   0.34$^B$    & $-$5.44  &   4.24E$-$6    &   17.2 & R   & I & 5.66E$-$4 \\
\object{R Cyg}  & S2.5,9e$-$S6,9e(Tc) & Mira &   0.55$^B$    & $-$5.42  &   9.04E$-$7    &   9.0 & R   & $-$ & 1.18E$-$3  \\
\object{chi Cyg}    & S6,2e$-$S10,4e/MSe & Mira &   0.18$^A$    & $-$5.39  &   8.69E$-$7    & 8.5   &   R   & I & 1.15E$-$4  \\
\object{T Cam}  & S4,7e$-$S8.5,8e & Mira &   0.50$^B$ & $-$5.22 & 8.91E$-$8    &   3.8   &   R & I & 6.73E$-$4 \\
\object{R Lyn} & S2.5,5e$-$S6,8e: & Mira & 0.95$^B$ & $-$5.19 & 3.90E$-$7    &   7.5   & R   & I & 3.70E$-$4 \\
\object{R Gem}  & S2,9e$-$S8,9e(Tc) & Mira &   0.66$^B$    & $-$5.23 &   3.91E$-$7    &   4.5 & R   & I & 2.67E$-$4  \\
\object{GI Lup} & S7,8e & Mira &   0.80$^B$    & $-$ &   7.20E$-$7    &   10.0 &   R   & I & 7.56E$-$4 \\
\object{WY Cas} & S6,5pe & Mira &   0.97$^B$    & $-$5.50 &   2.26E$-$6    &   13.5 &   R   & I & 1.56E$-$3 \\
\object{pi1 Gru}    & S5,7e & SRB &   0.16$^A$    & $-$5.75 &   2.57E$-$6 &   14.5 &   W   & I & 3.71E$-$4 \\
\object{ST Her} & M6$-$7IIIaS & SRB & 0.30$^A$ & $-$5.64 &   1.30E$-$7 &   8.5  &   R   & I & 4.62E$-$3 \\
\object{T Cet}  & M5$-$6SIIe & SRC &   0.27$^A$ & $-$5.63 & 4.93E$-$8    &   5.5 &   R & I & 2.08E$-$3 \\
\object{Y Lyn}  & M6SIb$-$II & SRC &   0.25$^A$    & $-$5.33 &   2.17E$-$7    &   7.5 & R & I & 7.83E$-$4  \\
\object{R And}  & S3,5e$-$S8,8e/M7e & Mira &   0.41$^B$    & $-$5.19 &   1.09E$-$6    & 8.3   &   R   & I & 3.67E$-$4 \\
\object{W And}  & S6,1e$-$S9,2e/M4$-$M1 & Mira &   0.38$^B$    & $-$5.27 &   2.79E$-$7    &   6.0 &   R   & I & 1.64E$-$3 \\
\object{RT Sco} & S7,2/M6e$-$M7e & Mira &   0.45$^B$ & $-$5.44 & 1.01E$-$6    &   11.0   & R   & I & 9.84E$-$4 \\
\object{RS Cnc} & M6eIb$-$II/S & SRC &   0.14$^A$    & $-$5.21  & 2.80E$-$7 &   6.8 &   L   & I & 6.78E$-$4 \\
\object{AA Cam} & M5/S & LB & 0.78$^A$    & $-$ & 3.83E$-$8    &   3.4   &   R & I & 2.10E$-$2 \\
\hline
\object{S Lyr}  & SCe & Mira &   2.27$^B$    & $-$5.50 & 5.44E$-$6    & 13.0  &   R   & I & 4.41E$-$4 \\
\object{TT Cen} & CSe & Mira &   1.39$^B$    & $-$5.48 &   5.17E$-$6    &   20.0 & R   & $-$ & 2.01E$-$3 \\
\object{ST Sgr} & C4,3e$-$S9,5e & Mira &   0.76$^B$ & $-$5.24 &   3.44E$-$7    &   6.0   & R   & I & 1.51E$-$3 \\
\object{UY Cen} & SC & SR &   0.69$^A$ & $-$6.05  & 1.70E$-$7    &   12.0 &   R & I & 2.35E$-$3 \\
\hline
\object{VX Aql} & C9,1p/M0ep & Mira & 1.99$^B$ & $-$5.87  & 3.51E$-$7    &   7.0 & R & I & 4.40E$-$3 \\
\hline
\end{tabular}
\tablefoot {\tablefoottext{a}{References for the distances are: \emph{A})~the revised Hipparcos catalogue \citep{vleu2007}; \emph{B})~the period-luminosity methods for the O-rich stars as used in Paper~II.}\\
\tablefoottext{b}{Bolometric Magnitudes are taken from Paper~II.}\\
\tablefoottext{c}{References for the mass loss rates (updated with our choice for distances) and for the outflow velocities are quoted~as: R~stands for \citet{ramstedt09}; W~is for \citet{winters03}; L~for \citet{loup}.}}
\vspace*{3.5mm}
\end{table}